Yale shooting problem - Revision history

en>The Anome: linked AAAI Classic Paper award

2015-01-08T16:25:28Z

← Older revision		Revision as of 18:25, 8 January 2015
Line 1:		Line 1:
	~~{{Starbox~~ begin		Hi there. Allow me begin by introducing the author, her title is Sophia Boon but she never really favored that title. To perform lacross is the factor I love most of all. Mississippi is exactly where his house is. My working day occupation is an invoicing officer but I've currently utilized for another 1.<br><br>My web page [http://www.youronlinepublishers.com/authWiki/AdolphvhBladenqq clairvoyants]
	~~\| name = Omega Andromedae~~
	}}
	~~{{Starbox image~~
	~~\| image =~~
	~~<div style="position: relative">[[File:Andromeda IAU.svg\|250px\|alt=Diagram showing star positions and boundaries of~~ the ~~Andromeda constellation and its surroundings]]~~
	~~<div style="position: absolute; left: 34.3%; top: 32.6%;">[[File:Cercle rouge 100%.svg\|12px]]</div>~~
	~~</div>~~
	~~\| caption = Location of ω Andromedae (circled)~~
	}}
	~~{{Starbox observe~~
	~~\| epoch = J2000~~
	~~\| ra = {{RA\|01\|27\|39.38177}}<ref name=aaa474_2_653/>~~
	~~\| dec = {{DEC\|+45\|24\|24.0727}}<ref name=aaa474_2_653/>~~
	~~\| appmag_v = +4.83<ref name=aaa418_989/><ref name=clpl4_99/>~~
	~~\| constell = [[Andromeda (constellation)\|Andromeda]]~~
	}}
	~~{{Starbox character~~
	~~\| class = F5 IVe<ref name=SIMBAD/>~~
	~~\| b-v = +0.42<ref name=clpl4_99/>~~
	~~\| u-b = +0.00<ref name=clpl4_99/>~~
	~~\| variable =~~
	}}
	~~{{Starbox astrometry~~
	~~\| radial_v = +14.7<ref name=aaa418_989/>~~
	~~\| prop_mo_ra = +356.99<ref name=aaa474_2_653/>~~
	~~\| prop_mo_dec = –109.40<ref name=aaa474_2_653/>~~
	~~\| parallax = 34.94~~
	~~\| p_error = 0.31~~
	~~\| parallax_footnote = <ref name=aaa474_2_653/>~~
	~~\| absmag_v = +2.57<ref name=aaa418_989/>~~
	}}
	~~{{Starbox detail~~
	~~\| mass =~~
	~~\| radius = 2.2<ref name=lang2006/>~~
	~~\| luminosity = 7.1<ref name=aaa405_723/>~~
	~~\| temperature = 6~~,~~628<ref name=aaa405_723/>~~
	~~\| metal_fe = –0.16<ref name=aaa418_989/>~~
	~~\| rotational_velocity = 57.1<ref name=aaa493_3_1099/>~~
	~~\| age_gyr = 2.1<ref name=aaa418_989/>~~
	}}
	~~{{Starbox catalog~~
	\| names= 48 Andromedae, [[Star catalogue#BD.2FCD.2FCPD\|BD]]+44°307, [[FK5]] 1040, [[Henry Draper Catalogue\|HD]] 8799, [[Hipparcos catalogue\|HIP]] 6813, [[Star catalogue#BS, BSC, HR\|HR]] 417, [[Star catalogue#SAO\|SAO]] 37228.<ref name=SIMBAD/>
	}}
	~~{{Starbox reference~~
	~~\| Simbad=HD+8799~~
	}}
	~~{{Starbox end}}~~

	~~'''Omega Andromedae''' (ω And, ω Andromedae)~~ is ~~the [[Bayer designation]] for a [[binary star]]<ref name=apj698_1_28/> system in the northern [[constellation]] of [[Andromeda (constellation)\|Andromeda]]~~. ~~Based upon [[parallax]] measurements made during the [[Hipparcos]] mission, this system~~ is located at a distance of approximately {{Convert\|93.3\|ly\|pc\|abbr=off\|lk=on}} from [[Earth]]. The [[apparent visual magnitude]] of Omega Andromedae is +4.83,<ref name=aaa418_989/> which makes it bright enough to be seen with the ~~naked eye.~~

	~~The primary component~~ of ~~this system has a [[stellar classification]] of F5 IVe~~.~~<ref name=SIMBAD/> The IV [[luminosity class]] indicates that it~~ is ~~probably a [[subgiant star]] that~~ is ~~in the process of [[stellar evolution\|evolving]] away from the [[main sequence]] as the supply of hydrogen at its core becomes exhausted~~. ~~The measured [[angular diameter]] of the primary star~~ is {{nowrap\|0.70 ± 0.03 [[milliarcsecond\|mas]]}}.<ref name=aaa431_773/> At the estimated distance of this system, this yields a physical size of about 2.2 times the [[Solar radius\|radius of the Sun]].<ref name=lang2006/> It is emitting about seven times the luminosity of the Sun from its [[stellar atmosphere\|outer atmosphere]] at an ~~[[effective temperature]] of 6,628 K.<ref name=aaa405_723/> This heat gives it the yellow-white hued glow of an [[F-type star]].<ref name=csiro/>~~

	In 2008, the companion star was resolved using [[adaptive optics]] at the [[Lick Observatory]]. Subsequent observations showed the magnitude difference between the two stars is 3.65 ± 0.03 and they are separated by 0.669 [[arcsecond]]s.<ref name=apj698_1_28/>

	~~==References==~~
	~~{{Reflist\|refs=~~

	<ref name=aaa474_2_653>{{citation \| first=F. \| last=van Leeuwen \|date=November 2007 \| title=Validation of the new Hipparcos reduction \| journal=Astronomy and Astrophysics \| volume=474 \| issue=2 \| pages=653–664 \| bibcode=2007A&A...474..653V \| doi=10.1051/0004-6361:20078357 \| postscript=. \|arxiv = 0708.1752 }}</ref>

	<ref name=aaa418_989>{{citation \| title=The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ˜14 000 F and G dwarfs \| display-authors=1 \| last1=Nordström \| first1=B. \| last2=Mayor \| first2=M. \| last3=Andersen \| first3=J. \| last4=Holmberg \| first4=J. \| last5=Pont \| first5=F. \| last6=Jørgensen \| first6=B. R. \| last7=Olsen \| first7=E. H. \| last8=Udry \| first8=S. \| last9=Mowlavi \| first9=N. \| journal=Astronomy and Astrophysics \| volume=418 \| pages=989–1019 \|date=May 2004 \| doi=10.1051/0004-6361:20035959 \| bibcode=2004A&A...418..989N \| arxiv=astro-ph/0405198 \| postscript=. }}</ref>

	~~<ref name=aaa493_3_1099>{{citation \| last1=Schröder \| first1=C. \| last2=Reiners \| first2=A. \| last3=Schmitt \| first3=J. H. M. M. \| title=Ca II HK emission in rapidly rotating stars. Evidence~~ for an onset of the solar-type dynamo \| journal=Astronomy and Astrophysics \| volume=493 \| issue=3 \| pages=1099–1107 \|date=January 2009 \| doi=10.1051/0004-6361:200810377 \| bibcode=2009A&A...493.1099S \| postscript=. }}</ref>

	<ref name=clpl4_99>{{citation \| display-authors=1 \| last1=Johnson \| first1=H. L. \| last2=Iriarte \| first2=B. \| last3=Mitchell \| first3=R. I. \| last4=Wisniewskj \| first4=W. Z. \| title=UBVRIJKL photometry of the bright stars \| journal=Communications of the Lunar and Planetary Laboratory \| volume=4 \| issue=99 \| year=1966 \| bibcode=1966CoLPL...4...99J \| postscript=. }}</ref>

	<ref name=SIMBAD>{{citation \| title=LTT 10517 -- High proper-motion Star \| work=SIMBAD Astronomical Object Database \| publisher=Centre de Données astronomiques de Strasbourg \| url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Omega+Andromedae \| accessdate=2012-06-26 \| postscript=. }}</ref>

	<ref name=apj698_1_28>{{citation \| last1=Gladysz \| first1=Szymon \| last2=Christou \| first2=Julian C. \| title=Reference-Less Detection, Astrometry, and Photometry of Faint Companions with Adaptive Optics \| journal=The Astrophysical Journal \| volume=698 \| issue=1 ~~\| pages=28–42 \|date=June 2009 \| doi=10~~.~~1088/0004-637X/698/1/28 \| bibcode=2009ApJ...698...28G \| postscript=. \|arxiv = 0805.1870 }}~~<~~/ref~~>

	<~~ref name=aaa405_723~~>{{citation \| display-authors=1 \| last1=do Nascimento \| first1=J. D., Jr. \| last2=Canto Martins \| first2=B. L. \| last3=Melo \| first3=C. H. F. \| last4=Porto de Mello \| first4=G. \| last5=De Medeiros \| first5=J. R. \| title=On the link between rotation, chromospheric activity and Li abundance in subgiant stars \| journal=Astronomy and Astrophysics \| volume=405 \| pages=723–731 \|date=July 2003 \| doi=10.1051/0004-6361:20030633 \| bibcode=2003A&A...405..723D \| arxiv=astro-ph/0307196 \| postscript=. }}</ref>

	<ref name=aaa431_773>{{citation \| last1=Richichi \| pages=A. \| last2=Percheron \| first2=I. \| last3=Khristoforova \| first3=M. \| title=CHARM2: An updated Catalog of High Angular Resolution Measurements \| journal=Astronomy and Astrophysics \| volume=431 \| pages=773–777 \|date=February 2005 \| doi=10.1051/0004-6361:20042039 \| bibcode=2005A&A...431..773R }}</ref>

	<ref name=lang2006>{{citation \| first1=Kenneth R. \| last1=Lang \| title=Astrophysical formulae \| volume=1 \| series=Astronomy and astrophysics library \| edition=3 \| publisher=Birkhäuser \| year=2006 \| isbn=3-540-29692-1 \| url=http://books.google.com/books?id=OvTjLcQ4MCQC&pg=PA41 }}. The radius (R<sub>*</sub>) is given by:
	:<math>\begin{align} 2\cdot R_*
	~~& = \frac{(28.6\cdot 0.70\cdot 10^{-3})\ \text{AU}}{0.0046491\ \text{AU}/R_{\bigodot}} \\~~
	~~& \approx 4.31\cdot R_{\bigodot}~~
	~~\end{align}</math></ref>~~

	<ref name=csiro>{{citation \| title=The Colour of Stars \| date=December 21, 2004 \| work=Australia Telescope, Outreach and Education \| publisher=Commonwealth Scientific and Industrial Research Organisation \| url=http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html \| accessdate=2012-01-16 \| postscript=. }}</ref>

	}}

	~~==External links==~~
	* [http://aladin.u-strasbg.fr/AladinPreview?-c=NLTT++4832&ident=NLTT++4832&submit=Aladin+previewer Image ω Andromedae]
	* [http://www.~~site~~.~~uottawa.ca:4321~~/~~astronomy~~/~~index.html#highpropermotionstar High proper-motion Star]~~

	~~{{Stars of Andromeda}}~~

	~~[[Category:Henry Draper Catalogue objects]]~~
	~~[[Category:Bayer objects\|Andromedae, Omega]]~~
	~~[[Category:Flamsteed objects\|Andromedae, 48]]~~
	~~[[Category:Andromeda (constellation)]]~~
	~~[[Category:F-type subgiants]~~]

en>Pinethicket: Reverted to revision 485186817 by Vlifschitz (talk): Last clean version. (TW)

2013-11-25T19:10:40Z

Reverted to revision 485186817 by Vlifschitz (talk): Last clean version. (TW)

← Older revision		Revision as of 21:10, 25 November 2013
Line 1:		Line 1:
	~~Hello~~, my name is ~~Andrew and my spouse doesn't like~~ it at ~~all~~. ~~My wife~~ and ~~I reside~~ in ~~Kentucky~~. ~~Doing ballet is some thing she would never give up~~. I ~~am an invoicing officer~~ and ~~I'll be promoted quickly~~.<br><br>~~Feel free to surf to my web~~-~~site~~: ~~[https~~://~~www~~-~~ocl~~.~~gist~~.ac.kr/work/xe/?~~document_srl~~=~~605236 certified psychics~~]		{{Starbox begin
			\| name = Omega Andromedae
			}}
			{{Starbox image
			\| image =
			<div style="position: relative">[[File:Andromeda IAU.svg\|250px\|alt=Diagram showing star positions and boundaries of the Andromeda constellation and its surroundings]]
			<div style="position: absolute; left: 34.3%; top: 32.6%;">[[File:Cercle rouge 100%.svg\|12px]]</div>
			</div>
			\| caption = Location of ω Andromedae (circled)
			}}
			{{Starbox observe
			\| epoch = J2000
			\| ra = {{RA\|01\|27\|39.38177}}<ref name=aaa474_2_653/>
			\| dec = {{DEC\|+45\|24\|24.0727}}<ref name=aaa474_2_653/>
			\| appmag_v = +4.83<ref name=aaa418_989/><ref name=clpl4_99/>
			\| constell = [[Andromeda (constellation)\|Andromeda]]
			}}
			{{Starbox character
			\| class = F5 IVe<ref name=SIMBAD/>
			\| b-v = +0.42<ref name=clpl4_99/>
			\| u-b = +0.00<ref name=clpl4_99/>
			\| variable =
			}}
			{{Starbox astrometry
			\| radial_v = +14.7<ref name=aaa418_989/>
			\| prop_mo_ra = +356.99<ref name=aaa474_2_653/>
			\| prop_mo_dec = –109.40<ref name=aaa474_2_653/>
			\| parallax = 34.94
			\| p_error = 0.31
			\| parallax_footnote = <ref name=aaa474_2_653/>
			\| absmag_v = +2.57<ref name=aaa418_989/>
			}}
			{{Starbox detail
			\| mass =
			\| radius = 2.2<ref name=lang2006/>
			\| luminosity = 7.1<ref name=aaa405_723/>
			\| temperature = 6,628<ref name=aaa405_723/>
			\| metal_fe = –0.16<ref name=aaa418_989/>
			\| rotational_velocity = 57.1<ref name=aaa493_3_1099/>
			\| age_gyr = 2.1<ref name=aaa418_989/>
			}}
			{{Starbox catalog
			\| names= 48 Andromedae, [[Star catalogue#BD.2FCD.2FCPD\|BD]]+44°307, [[FK5]] 1040, [[Henry Draper Catalogue\|HD]] 8799, [[Hipparcos catalogue\|HIP]] 6813, [[Star catalogue#BS, BSC, HR\|HR]] 417, [[Star catalogue#SAO\|SAO]] 37228.<ref name=SIMBAD/>
			}}
			{{Starbox reference
			\| Simbad=HD+8799
			}}
			{{Starbox end}}

			'''Omega Andromedae''' (ω And, ω Andromedae) is the [[Bayer designation]] for a [[binary star]]<ref name=apj698_1_28/> system in the northern [[constellation]] of [[Andromeda (constellation)\|Andromeda]]. Based upon [[parallax]] measurements made during the [[Hipparcos]] mission, this system is located at a distance of approximately {{Convert\|93.3\|ly\|pc\|abbr=off\|lk=on}} from [[Earth]]. The [[apparent visual magnitude]] of Omega Andromedae is +4.83,<ref name=aaa418_989/> which makes it bright enough to be seen with the naked eye.

			The primary component of this system has a [[stellar classification]] of F5 IVe.<ref name=SIMBAD/> The IV [[luminosity class]] indicates that it is probably a [[subgiant star]] that is in the process of [[stellar evolution\|evolving]] away from the [[main sequence]] as the supply of hydrogen at its core becomes exhausted. The measured [[angular diameter]] of the primary star is {{nowrap\|0.70 ± 0.03 [[milliarcsecond\|mas]]}}.<ref name=aaa431_773/> At the estimated distance of this system, this yields a physical size of about 2.2 times the [[Solar radius\|radius of the Sun]].<ref name=lang2006/> It is emitting about seven times the luminosity of the Sun from its [[stellar atmosphere\|outer atmosphere]] at an [[effective temperature]] of 6,628 K.<ref name=aaa405_723/> This heat gives it the yellow-white hued glow of an [[F-type star]].<ref name=csiro/>

			In 2008, the companion star was resolved using [[adaptive optics]] at the [[Lick Observatory]]. Subsequent observations showed the magnitude difference between the two stars is 3.65 ± 0.03 and they are separated by 0.669 [[arcsecond]]s.<ref name=apj698_1_28/>

			==References==
			{{Reflist\|refs=

			<ref name=aaa474_2_653>{{citation \| first=F. \| last=van Leeuwen \|date=November 2007 \| title=Validation of the new Hipparcos reduction \| journal=Astronomy and Astrophysics \| volume=474 \| issue=2 \| pages=653–664 \| bibcode=2007A&A...474..653V \| doi=10.1051/0004-6361:20078357 \| postscript=. \|arxiv = 0708.1752 }}</ref>

			<ref name=aaa418_989>{{citation \| title=The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ˜14 000 F and G dwarfs \| display-authors=1 \| last1=Nordström \| first1=B. \| last2=Mayor \| first2=M. \| last3=Andersen \| first3=J. \| last4=Holmberg \| first4=J. \| last5=Pont \| first5=F. \| last6=Jørgensen \| first6=B. R. \| last7=Olsen \| first7=E. H. \| last8=Udry \| first8=S. \| last9=Mowlavi \| first9=N. \| journal=Astronomy and Astrophysics \| volume=418 \| pages=989–1019 \|date=May 2004 \| doi=10.1051/0004-6361:20035959 \| bibcode=2004A&A...418..989N \| arxiv=astro-ph/0405198 \| postscript=. }}</ref>

			<ref name=aaa493_3_1099>{{citation \| last1=Schröder \| first1=C. \| last2=Reiners \| first2=A. \| last3=Schmitt \| first3=J. H. M. M. \| title=Ca II HK emission in rapidly rotating stars. Evidence for an onset of the solar-type dynamo \| journal=Astronomy and Astrophysics \| volume=493 \| issue=3 \| pages=1099–1107 \|date=January 2009 \| doi=10.1051/0004-6361:200810377 \| bibcode=2009A&A...493.1099S \| postscript=. }}</ref>

			<ref name=clpl4_99>{{citation \| display-authors=1 \| last1=Johnson \| first1=H. L. \| last2=Iriarte \| first2=B. \| last3=Mitchell \| first3=R. I. \| last4=Wisniewskj \| first4=W. Z. \| title=UBVRIJKL photometry of the bright stars \| journal=Communications of the Lunar and Planetary Laboratory \| volume=4 \| issue=99 \| year=1966 \| bibcode=1966CoLPL...4...99J \| postscript=. }}</ref>

			<ref name=SIMBAD>{{citation \| title=LTT 10517 -- High proper-motion Star \| work=SIMBAD Astronomical Object Database \| publisher=Centre de Données astronomiques de Strasbourg \| url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Omega+Andromedae \| accessdate=2012-06-26 \| postscript=. }}</ref>

			<ref name=apj698_1_28>{{citation \| last1=Gladysz \| first1=Szymon \| last2=Christou \| first2=Julian C. \| title=Reference-Less Detection, Astrometry, and Photometry of Faint Companions with Adaptive Optics \| journal=The Astrophysical Journal \| volume=698 \| issue=1 \| pages=28–42 \|date=June 2009 \| doi=10.1088/0004-637X/698/1/28 \| bibcode=2009ApJ...698...28G \| postscript=. \|arxiv = 0805.1870 }}</ref>

			<ref name=aaa405_723>{{citation \| display-authors=1 \| last1=do Nascimento \| first1=J. D., Jr. \| last2=Canto Martins \| first2=B. L. \| last3=Melo \| first3=C. H. F. \| last4=Porto de Mello \| first4=G. \| last5=De Medeiros \| first5=J. R. \| title=On the link between rotation, chromospheric activity and Li abundance in subgiant stars \| journal=Astronomy and Astrophysics \| volume=405 \| pages=723–731 \|date=July 2003 \| doi=10.1051/0004-6361:20030633 \| bibcode=2003A&A...405..723D \| arxiv=astro-ph/0307196 \| postscript=. }}</ref>

			<ref name=aaa431_773>{{citation \| last1=Richichi \| pages=A. \| last2=Percheron \| first2=I. \| last3=Khristoforova \| first3=M. \| title=CHARM2: An updated Catalog of High Angular Resolution Measurements \| journal=Astronomy and Astrophysics \| volume=431 \| pages=773–777 \|date=February 2005 \| doi=10.1051/0004-6361:20042039 \| bibcode=2005A&A...431..773R }}</ref>

			<ref name=lang2006>{{citation \| first1=Kenneth R. \| last1=Lang \| title=Astrophysical formulae \| volume=1 \| series=Astronomy and astrophysics library \| edition=3 \| publisher=Birkhäuser \| year=2006 \| isbn=3-540-29692-1 \| url=http://books.google.com/books?id=OvTjLcQ4MCQC&pg=PA41 }}. The radius (R<sub>*</sub>) is given by:
			:<math>\begin{align} 2\cdot R_*
			& = \frac{(28.6\cdot 0.70\cdot 10^{-3})\ \text{AU}}{0.0046491\ \text{AU}/R_{\bigodot}} \\
			& \approx 4.31\cdot R_{\bigodot}
			\end{align}</math></ref>

			<ref name=csiro>{{citation \| title=The Colour of Stars \| date=December 21, 2004 \| work=Australia Telescope, Outreach and Education \| publisher=Commonwealth Scientific and Industrial Research Organisation \| url=http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html \| accessdate=2012-01-16 \| postscript=. }}</ref>

			}}

			==External links==
			* [http://aladin.u-strasbg.fr/AladinPreview?-c=NLTT++4832&ident=NLTT++4832&submit=Aladin+previewer Image ω Andromedae]
			* [http://www.site.uottawa.ca:4321/astronomy/index.html#highpropermotionstar High proper-motion Star]

			{{Stars of Andromeda}}

			[[Category:Henry Draper Catalogue objects]]
			[[Category:Bayer objects\|Andromedae, Omega]]
			[[Category:Flamsteed objects\|Andromedae, 48]]
			[[Category:Andromeda (constellation)]]
			[[Category:F-type subgiants]]

en>Vlifschitz: Classic paper award

2012-04-02T16:51:44Z

Classic paper award

New page

Hello, my name is Andrew and my spouse doesn't like it at all. My wife and I reside in Kentucky. Doing ballet is some thing she would never give up. I am an invoicing officer and I'll be promoted quickly.<br><br>Feel free to surf to my web-site: [https://www-ocl.gist.ac.kr/work/xe/?document_srl=605236 certified psychics]

← Older revision		Revision as of 18:25, 8 January 2015
Line 1:		Line 1:
	~~{{Starbox~~ begin		Hi there. Allow me begin by introducing the author, her title is Sophia Boon but she never really favored that title. To perform lacross is the factor I love most of all. Mississippi is exactly where his house is. My working day occupation is an invoicing officer but I've currently utilized for another 1.<br><br>My web page [http://www.youronlinepublishers.com/authWiki/AdolphvhBladenqq clairvoyants]
	~~\| name = Omega Andromedae~~
	}}
	~~{{Starbox image~~
	~~\| image =~~
	~~<div style="position: relative">[[File:Andromeda IAU.svg\|250px\|alt=Diagram showing star positions and boundaries of~~ the ~~Andromeda constellation and its surroundings]]~~
	~~<div style="position: absolute; left: 34.3%; top: 32.6%;">[[File:Cercle rouge 100%.svg\|12px]]</div>~~
	~~</div>~~
	~~\| caption = Location of ω Andromedae (circled)~~
	}}
	~~{{Starbox observe~~
	~~\| epoch = J2000~~
	~~\| ra = {{RA\|01\|27\|39.38177}}<ref name=aaa474_2_653/>~~
	~~\| dec = {{DEC\|+45\|24\|24.0727}}<ref name=aaa474_2_653/>~~
	~~\| appmag_v = +4.83<ref name=aaa418_989/><ref name=clpl4_99/>~~
	~~\| constell = [[Andromeda (constellation)\|Andromeda]]~~
	}}
	~~{{Starbox character~~
	~~\| class = F5 IVe<ref name=SIMBAD/>~~
	~~\| b-v = +0.42<ref name=clpl4_99/>~~
	~~\| u-b = +0.00<ref name=clpl4_99/>~~
	~~\| variable =~~
	}}
	~~{{Starbox astrometry~~
	~~\| radial_v = +14.7<ref name=aaa418_989/>~~
	~~\| prop_mo_ra = +356.99<ref name=aaa474_2_653/>~~
	~~\| prop_mo_dec = –109.40<ref name=aaa474_2_653/>~~
	~~\| parallax = 34.94~~
	~~\| p_error = 0.31~~
	~~\| parallax_footnote = <ref name=aaa474_2_653/>~~
	~~\| absmag_v = +2.57<ref name=aaa418_989/>~~
	}}
	~~{{Starbox detail~~
	~~\| mass =~~
	~~\| radius = 2.2<ref name=lang2006/>~~
	~~\| luminosity = 7.1<ref name=aaa405_723/>~~
	~~\| temperature = 6~~,~~628<ref name=aaa405_723/>~~
	~~\| metal_fe = –0.16<ref name=aaa418_989/>~~
	~~\| rotational_velocity = 57.1<ref name=aaa493_3_1099/>~~
	~~\| age_gyr = 2.1<ref name=aaa418_989/>~~
	}}
	~~{{Starbox catalog~~
	\| names= 48 Andromedae, [[Star catalogue#BD.2FCD.2FCPD\|BD]]+44°307, [[FK5]] 1040, [[Henry Draper Catalogue\|HD]] 8799, [[Hipparcos catalogue\|HIP]] 6813, [[Star catalogue#BS, BSC, HR\|HR]] 417, [[Star catalogue#SAO\|SAO]] 37228.<ref name=SIMBAD/>
	}}
	~~{{Starbox reference~~
	~~\| Simbad=HD+8799~~
	}}
	~~{{Starbox end}}~~

	~~'''Omega Andromedae''' (ω And, ω Andromedae)~~ is ~~the [[Bayer designation]] for a [[binary star]]<ref name=apj698_1_28/> system in the northern [[constellation]] of [[Andromeda (constellation)\|Andromeda]]~~. ~~Based upon [[parallax]] measurements made during the [[Hipparcos]] mission, this system~~ is located at a distance of approximately {{Convert\|93.3\|ly\|pc\|abbr=off\|lk=on}} from [[Earth]]. The [[apparent visual magnitude]] of Omega Andromedae is +4.83,<ref name=aaa418_989/> which makes it bright enough to be seen with the ~~naked eye.~~

	~~The primary component~~ of ~~this system has a [[stellar classification]] of F5 IVe~~.~~<ref name=SIMBAD/> The IV [[luminosity class]] indicates that it~~ is ~~probably a [[subgiant star]] that~~ is ~~in the process of [[stellar evolution\|evolving]] away from the [[main sequence]] as the supply of hydrogen at its core becomes exhausted~~. ~~The measured [[angular diameter]] of the primary star~~ is {{nowrap\|0.70 ± 0.03 [[milliarcsecond\|mas]]}}.<ref name=aaa431_773/> At the estimated distance of this system, this yields a physical size of about 2.2 times the [[Solar radius\|radius of the Sun]].<ref name=lang2006/> It is emitting about seven times the luminosity of the Sun from its [[stellar atmosphere\|outer atmosphere]] at an ~~[[effective temperature]] of 6,628 K.<ref name=aaa405_723/> This heat gives it the yellow-white hued glow of an [[F-type star]].<ref name=csiro/>~~

	In 2008, the companion star was resolved using [[adaptive optics]] at the [[Lick Observatory]]. Subsequent observations showed the magnitude difference between the two stars is 3.65 ± 0.03 and they are separated by 0.669 [[arcsecond]]s.<ref name=apj698_1_28/>

	~~==References==~~
	~~{{Reflist\|refs=~~

	<ref name=aaa474_2_653>{{citation \| first=F. \| last=van Leeuwen \|date=November 2007 \| title=Validation of the new Hipparcos reduction \| journal=Astronomy and Astrophysics \| volume=474 \| issue=2 \| pages=653–664 \| bibcode=2007A&A...474..653V \| doi=10.1051/0004-6361:20078357 \| postscript=. \|arxiv = 0708.1752 }}</ref>

	<ref name=aaa418_989>{{citation \| title=The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ˜14 000 F and G dwarfs \| display-authors=1 \| last1=Nordström \| first1=B. \| last2=Mayor \| first2=M. \| last3=Andersen \| first3=J. \| last4=Holmberg \| first4=J. \| last5=Pont \| first5=F. \| last6=Jørgensen \| first6=B. R. \| last7=Olsen \| first7=E. H. \| last8=Udry \| first8=S. \| last9=Mowlavi \| first9=N. \| journal=Astronomy and Astrophysics \| volume=418 \| pages=989–1019 \|date=May 2004 \| doi=10.1051/0004-6361:20035959 \| bibcode=2004A&A...418..989N \| arxiv=astro-ph/0405198 \| postscript=. }}</ref>

	~~<ref name=aaa493_3_1099>{{citation \| last1=Schröder \| first1=C. \| last2=Reiners \| first2=A. \| last3=Schmitt \| first3=J. H. M. M. \| title=Ca II HK emission in rapidly rotating stars. Evidence~~ for an onset of the solar-type dynamo \| journal=Astronomy and Astrophysics \| volume=493 \| issue=3 \| pages=1099–1107 \|date=January 2009 \| doi=10.1051/0004-6361:200810377 \| bibcode=2009A&A...493.1099S \| postscript=. }}</ref>

	<ref name=clpl4_99>{{citation \| display-authors=1 \| last1=Johnson \| first1=H. L. \| last2=Iriarte \| first2=B. \| last3=Mitchell \| first3=R. I. \| last4=Wisniewskj \| first4=W. Z. \| title=UBVRIJKL photometry of the bright stars \| journal=Communications of the Lunar and Planetary Laboratory \| volume=4 \| issue=99 \| year=1966 \| bibcode=1966CoLPL...4...99J \| postscript=. }}</ref>

	<ref name=SIMBAD>{{citation \| title=LTT 10517 -- High proper-motion Star \| work=SIMBAD Astronomical Object Database \| publisher=Centre de Données astronomiques de Strasbourg \| url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Omega+Andromedae \| accessdate=2012-06-26 \| postscript=. }}</ref>

	<ref name=apj698_1_28>{{citation \| last1=Gladysz \| first1=Szymon \| last2=Christou \| first2=Julian C. \| title=Reference-Less Detection, Astrometry, and Photometry of Faint Companions with Adaptive Optics \| journal=The Astrophysical Journal \| volume=698 \| issue=1 ~~\| pages=28–42 \|date=June 2009 \| doi=10~~.~~1088/0004-637X/698/1/28 \| bibcode=2009ApJ...698...28G \| postscript=. \|arxiv = 0805.1870 }}~~<~~/ref~~>

	<~~ref name=aaa405_723~~>{{citation \| display-authors=1 \| last1=do Nascimento \| first1=J. D., Jr. \| last2=Canto Martins \| first2=B. L. \| last3=Melo \| first3=C. H. F. \| last4=Porto de Mello \| first4=G. \| last5=De Medeiros \| first5=J. R. \| title=On the link between rotation, chromospheric activity and Li abundance in subgiant stars \| journal=Astronomy and Astrophysics \| volume=405 \| pages=723–731 \|date=July 2003 \| doi=10.1051/0004-6361:20030633 \| bibcode=2003A&A...405..723D \| arxiv=astro-ph/0307196 \| postscript=. }}</ref>

	<ref name=aaa431_773>{{citation \| last1=Richichi \| pages=A. \| last2=Percheron \| first2=I. \| last3=Khristoforova \| first3=M. \| title=CHARM2: An updated Catalog of High Angular Resolution Measurements \| journal=Astronomy and Astrophysics \| volume=431 \| pages=773–777 \|date=February 2005 \| doi=10.1051/0004-6361:20042039 \| bibcode=2005A&A...431..773R }}</ref>

	<ref name=lang2006>{{citation \| first1=Kenneth R. \| last1=Lang \| title=Astrophysical formulae \| volume=1 \| series=Astronomy and astrophysics library \| edition=3 \| publisher=Birkhäuser \| year=2006 \| isbn=3-540-29692-1 \| url=http://books.google.com/books?id=OvTjLcQ4MCQC&pg=PA41 }}. The radius (R<sub>*</sub>) is given by:
	:<math>\begin{align} 2\cdot R_*
	~~& = \frac{(28.6\cdot 0.70\cdot 10^{-3})\ \text{AU}}{0.0046491\ \text{AU}/R_{\bigodot}} \\~~
	~~& \approx 4.31\cdot R_{\bigodot}~~
	~~\end{align}</math></ref>~~

	<ref name=csiro>{{citation \| title=The Colour of Stars \| date=December 21, 2004 \| work=Australia Telescope, Outreach and Education \| publisher=Commonwealth Scientific and Industrial Research Organisation \| url=http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html \| accessdate=2012-01-16 \| postscript=. }}</ref>

	}}

	~~==External links==~~
	* [http://aladin.u-strasbg.fr/AladinPreview?-c=NLTT++4832&ident=NLTT++4832&submit=Aladin+previewer Image ω Andromedae]
	* [http://www.~~site~~.~~uottawa.ca:4321~~/~~astronomy~~/~~index.html#highpropermotionstar High proper-motion Star]~~

	~~{{Stars of Andromeda}}~~

	~~[[Category:Henry Draper Catalogue objects]]~~
	~~[[Category:Bayer objects\|Andromedae, Omega]]~~
	~~[[Category:Flamsteed objects\|Andromedae, 48]]~~
	~~[[Category:Andromeda (constellation)]]~~
	~~[[Category:F-type subgiants]~~]