NGC 4314 - Revision history

wikademia>Wikademia at 20:27, 11 April 2009

2009-04-11T20:27:12Z

← Older revision		Revision as of 20:27, 11 April 2009
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	'''NGC 4314''' is a [[barred spiral galaxy]] approximately 40 million [[light-years]] away in the [[constellation~~]] [[~~Coma Berenices]]. Perhaps the most prominent and unusual feature is its "nuclear starbust ring." It is thought that this explosion of star formation has occurred over the past few millions of years. This time frame is remarkably short in astronomical terms because most [[main sequence]] stars have lifetimes of billions of years and their birth is not usually uniform throughout a galaxy. Further study will be required to understand more about the evolution of such ring structures in galaxies.		'''NGC 4314''' is a barred spiral galaxy approximately 40 million light-years away in the constellation Coma Berenices. Perhaps the most prominent and unusual feature is its "nuclear starbust ring." It is thought that this explosion of star formation has occurred over the past few millions of years. This time frame is remarkably short in astronomical terms because most main sequence stars have lifetimes of billions of years and their birth is not usually uniform throughout a galaxy. Further study will be required to understand more about the evolution of such ring structures in galaxies.

	==External links==		==External links==
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	[[Category:UGC objects\|07443]]		[[Category:UGC objects\|07443]]
	[[Category:PGC objects\|40097]]		[[Category:PGC objects\|40097]]
			{{ntnes}}

2009-04-04T20:43:11Z

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 '''NGC 4314''' is a [[barred spiral galaxy]] approximately 40 million [[light-years]] away in the [[constellation]] [[Coma Berenices]].  Perhaps the most prominent and unusual feature is its "nuclear starbust ring."  It is thought that this explosion of star formation has occurred over the past few millions of years.  This time frame is remarkably short in astronomical terms because most  [[main sequence]] stars have lifetimes of billions of years and their birth is not usually uniform throughout a galaxy.  Further study will be required to understand more about the evolution of such ring structures in galaxies.
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 * [http://mcdonaldobservatory.org/news/releases/2002/0409.html '''McDonald Observatory''': 9 April 2002 News Release]
 * [http://www.spacetelescope.org/bin/images.pl?searchtype=freesearch&string=4314 '''ESA/Hubble''' NGC 4314]
 [[Category:Spiral galaxies]]
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 [[Category:UGC objects|07443]]
 [[Category:PGC objects|40097]]

2009-04-04T05:23:49Z

27 revisions

← Older revision	Revision as of 05:23, 4 April 2009
(No difference)

2009-03-02T17:42:10Z

robot Adding: it:NGC 4314

2008-12-30T21:56:50Z

Units/dates/other

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	\| dec = {{DEC\|+29\|53\|43}}<ref name="ned" />		\| dec = {{DEC\|+29\|53\|43}}<ref name="ned" />
	\| dist_ly =		\| dist_ly =
	\| z = 963 ± 5 ~~[[kilometer\|~~km]]/[[second\|s]]<ref name="ned" />		\| z = 963 ± 5 km/[[second\|s]]<ref name="ned" />
	\| appmag_v = 11.4<ref name="ned" />		\| appmag_v = 11.4<ref name="ned" />
	\| size_v = 4′.2 × 3′.7<ref name="ned" />		\| size_v = 4′.2 × 3′.7<ref name="ned" />

2008-07-15T21:47:06Z

Resolving redirect

← Older revision		Revision as of 21:47, 15 July 2008
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	{{Galaxy		{{Infobox Galaxy
	\| name = [[New General Catalogue\|NGC]] 4314		\| name = [[New General Catalogue\|NGC]] 4314
	\| image = [[Image:NGC4314.jpg\|250px]]		\| image = [[Image:NGC4314.jpg\|250px]]

2008-07-05T13:02:39Z

clean up + reference formating fixes using AWB

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	==References==		==References==

	~~<div class="references-small"><references/></div>~~		{{reflist}}

	[[Category:Spiral galaxies]]		[[Category:Spiral galaxies]]

2008-02-01T05:59:54Z

caption

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	\| name = [[New General Catalogue\|NGC]] 4314		\| name = [[New General Catalogue\|NGC]] 4314
	\| image = [[Image:NGC4314.jpg\|250px]]		\| image = [[Image:NGC4314.jpg\|250px]]
	~~<small>~~A [[Hubble Space Telescope]] (HST) image of NGC 4314.~~<br/>Credit:~~ HST/[[NASA]]/[[ESA]]~~.</small>~~		\|caption= A [[Hubble Space Telescope]] (HST) image of NGC 4314.
			\| credit= HST/[[NASA]]/[[ESA]]
	\| epoch = [[J2000]]		\| epoch = [[J2000]]
	\| type = SB(rs)a<ref name="ned">{{cite web		\| type = SB(rs)a<ref name="ned">{{cite web

2007-11-11T02:53:07Z

Fix and format:units and/or dates.

← Older revision		Revision as of 02:53, 11 November 2007
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	\| z = 963 ± 5 [[kilometer\|km]]/[[second\|s]]<ref name="ned" />		\| z = 963 ± 5 [[kilometer\|km]]/[[second\|s]]<ref name="ned" />
	\| appmag_v = 11.4<ref name="ned" />		\| appmag_v = 11.4<ref name="ned" />
	\| size_v = 4′.2 ~~×~~ 3′.7<ref name="ned" />		\| size_v = 4′.2 × 3′.7<ref name="ned" />
	\| constellation name = [[Coma Berenices]]		\| constellation name = [[Coma Berenices]]
	\| notes =		\| notes =

2007-11-11T00:05:09Z

← Older revision		Revision as of 00:05, 11 November 2007
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	}}		}}

	'''NGC 4314''' is a [[barred spiral galaxy]] approximately 40 million [[light-years]] away in the [[constellation]] [[Coma Berenices]]. Perhaps the most prominent and unusual feature is its "nuclear starbust ring." It is thought that this explosion of star formation has occurred over the past few millions of years. This time frame is remarkably short in astronomical terms ~~due to the fact that~~ most [[main sequence]] stars have lifetimes of billions of years and their birth is not usually uniform throughout a galaxy. Further study will be required to understand more about the evolution of such ring structures in galaxies.		'''NGC 4314''' is a [[barred spiral galaxy]] approximately 40 million [[light-years]] away in the [[constellation]] [[Coma Berenices]]. Perhaps the most prominent and unusual feature is its "nuclear starbust ring." It is thought that this explosion of star formation has occurred over the past few millions of years. This time frame is remarkably short in astronomical terms because most [[main sequence]] stars have lifetimes of billions of years and their birth is not usually uniform throughout a galaxy. Further study will be required to understand more about the evolution of such ring structures in galaxies.

	==External links==		==External links==