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			{{short description\|Galaxy in the constellation Leo}}
	{{redirect\|M95}}		{{redirect\|M95}}
	{{Use dmy dates\|date=April ~~2012~~}}		{{Use dmy dates\|date=April 2021}}
	{{Infobox Galaxy		{{Infobox Galaxy
	\| name = ] 95		\| name = ] 95
	\| image = ~~Messier95~~ ~~spitzer~~.~~jpg~~		\| image = File:M95 - HST - Potw1841a.tiff
	\| image_size = ~~250px~~		\| image_size = 300px
	\| caption = ~~M95.~~ ~~Credit:~~ ]		\| caption = Hubble Space Telescope image of Messier 95
	\| epoch = ]		\| epoch = ]
	\| ra = {{RA\|10\|43\|57.7}}<ref name="ned">{{cite web		\| ra = {{RA\|10\|43\|57.7}}<ref name="ned">{{cite web
Line 11:		Line 12:
	\| work=Results for NGC 3351		\| work=Results for NGC 3351
	\| url=http://nedwww.ipac.caltech.edu/		\| url=http://nedwww.ipac.caltech.edu/
	\| ~~accessdate~~=2007-10-03}}</ref>		\| access-date=2007-10-03}}</ref>
	\| dec = {{DEC\|+11\|42\|14}}<ref name="ned" />		\| dec = {{DEC\|+11\|42\|14}}<ref name="ned" />
	\| constellation name = ]		\| constellation name = ]
	\| z = 778 ± 4 km/]<ref name="ned" />		\| z = 778 ± 4 km/]<ref name="ned" />
	\| dist_ly =32.6 ± 1.4 ] (10.0 ± 0.4 ])<ref name="jensenetal2003">		\| dist_ly =32.6 ± 1.4 ] (10.0 ± 0.4 ])<ref name="jensenetal2003">
	{{cite journal		{{cite journal
	\| author=Jensen, Joseph B. \| author2=Tonry, John L. \| author3=Barris, Brian J. \| author4=Thompson, Rodger I. \| author5=Liu, Michael C. \| author6=Rieke, Marcia J. \| author7=Ajhar, Edward A. \| author8=Blakeslee, John P.		\| author=Jensen, Joseph B. \| author2=Tonry, John L. \| author3=Barris, Brian J. \| author4=Thompson, Rodger I. \| author5=Liu, Michael C. \| author6=Rieke, Marcia J. \| author7=Ajhar, Edward A. \| author8=Blakeslee, John P.
	\| ~~displayauthors~~=4		\| display-authors=4
	\| date=2003		\| date=2003
	\| title=Measuring Distances and Probing the Unresolved Stellar Populations of Galaxies Using Infrared Surface Brightness Fluctuations		\| title=Measuring Distances and Probing the Unresolved Stellar Populations of Galaxies Using Infrared Surface Brightness Fluctuations
Line 25:		Line 26:
	\| bibcode=2003ApJ...583..712J		\| bibcode=2003ApJ...583..712J
	\| doi=10.1086/345430		\| doi=10.1086/345430
	\|arxiv = astro-ph/0210129 }}</ref>		\|arxiv = astro-ph/0210129 \| s2cid=551714 }}</ref>
	\| type = SB(r)b<ref name="ned" />		\| type = SB(r)b<ref name="ned" />
			\| appmag_v = 9.7<ref>{{cite web \|url=https://messier.seds.org/m/m095.html \|title=Messier 95 \|access-date=30 April 2022 \|website=SEDS Messier Catalog}}</ref>
	\| appmag_v = 11.4<ref name="ned" />
	\| size_v = 3′.1 × 2′.9<ref name="ned" />		\| size_v = 3′.1 × 2′.9<ref name="ned" />
	\| notes =		\| notes =
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	}}		}}

	'''Messier 95''', also known as '''M95''' or '''NGC 3351''', is a ] ~~located~~ about 38 million ]s away in the ] ] ]. It was discovered by ] in 1781, and catalogued by ~~fellow French astronomer~~ ] four days later. On 16 ~~March~~ ~~2012,~~ a ] was discovered ~~in M95~~.		'''Messier 95''', also known as '''M95''' or '''NGC 3351''', is a ] about 33 million ]s away in the ] ] ]. It was discovered by ] in 1781, and catalogued by compatriot ] four days later. In 2012 its most recent ] was discovered.

	The galaxy has a morphological classification of SB(r)b,<ref name="ned" /> with the SBb notation indicating it is a barred spiral with arms that are intermediate on the scale from tightly to loosely wound, and an '(r)' meaning an inner ring surrounds the bar.<ref name=Buta2007>{{citation		The galaxy has a morphological classification of SB(r)b,<ref name="ned" /> with the SBb notation indicating it is a barred spiral with arms that are intermediate on the scale from tightly to loosely wound, and an "(r)" meaning an inner ring surrounds the bar.<ref name=Buta2007>{{citation
	\| title=Atlas of Galaxies \| postscript=.		\| title=Atlas of Galaxies \| postscript=.
	\| display-authors=1 \| first1=Ronald J. \| last1=Buta		\| display-authors=1 \| first1=Ronald J. \| last1=Buta
	\| first2=Harold G. \| last2=Corwin \| first3=Stephen C. \| last3=Odewahn		\| first2=Harold G. \| last2=Corwin \| first3=Stephen C. \| last3=Odewahn
	\| publisher=Cambridge University Press		\| publisher=Cambridge University Press
	\| year=2007 \| isbn=~~0521820480~~ \| pages=1−25		\| year=2007 \| isbn=978-0521820486 \| pages=1−25
	\| url=https://books.google.com/books?id=g-P7dCbB5MEC&pg=PA1		\| url=https://books.google.com/books?id=g-P7dCbB5MEC&pg=PA1
	}}</ref> The latter is a ring-shaped, circumnuclear ] with a diameter of approximately {{Convert\|~~2000~~\|ly\|pc}}.<ref>{{cite journal		}}</ref> The latter is a ring-shaped, circumnuclear ] with a diameter of approximately {{Convert\|70,000\|ly\|pc}}.<ref>{{cite journal
	~~\| display-authors=5~~ \| first1=L. \| last1=Colina		\| first1=L. \| last1=Colina
	\| first2=M. L. \| last2=Garcia Vargas \| first3=J. M. \| last3=Mas-Hesse		\| first2=M. L. \| last2=Garcia Vargas \| first3=J. M. \| last3=Mas-Hesse
	\| first4=A. \| last4=Alberdi \| first5=A. \| last5=Krabbe \| date=1997		\| first4=A. \| last4=Alberdi \| first5=A. \| last5=Krabbe \| date=1997
Line 49:		Line 50:
	\| journal=] \| volume=484 \| issue=1		\| journal=] \| volume=484 \| issue=1
	\| pages=L41–L45 \| bibcode=1997ApJ...484L..41C \| doi=10.1086/310766		\| pages=L41–L45 \| bibcode=1997ApJ...484L..41C \| doi=10.1086/310766
	}}</ref> The spiral structure extends outward from the ring.<ref name=Buta2007/>		\| doi-access=free }}</ref> The spiral structure extends outward from the ring.<ref name=Buta2007/>

	~~The~~ ring structure of ~~M95 has a mass of~~ {{solar mass\|{{val\|3.5\|e=8}}\|link=yes}} in molecular gas and a star formation rate of {{solar mass\|0.38}} yr<sup>−1</sup>. The star formation is occurring in at least five regions with diameters between 100 and 150 pc that are composed of several star clusters ranging in size from 1.7 to 4.9 pc. These individual clusters contain {{Val\|1.8\|-\|8.7\|e=6\|u=solar_mass}} of stars, and may be on the path to forming ]s.<ref name=Haegele2007>{{citation		Its ring structure is about {{solar mass\|{{val\|3.5\|e=8}}\|link=yes}} (solar masses) in molecular gas and yields a star formation rate of {{solar mass\|0.38}} yr<sup>−1</sup>.{{efn\|meaning per year}} The star formation is occurring in at least five regions with diameters between 100 and 150 pc that are composed of several star clusters ranging in size from 1.7 to 4.9 pc. These individual clusters contain {{Val\|1.8\|-\|8.7\|e=6\|u=solar_mass}}{{efn\|1.8 to 8.7 million solar masses}} of stars, and may be on the path to forming ]s.<ref name=Haegele2007>{{citation
	\| title=Kinematics of gas and stars in the circumnuclear star-forming ring of NGC3351		\| title=Kinematics of gas and stars in the circumnuclear star-forming ring of NGC3351
	\| display-authors=1 \| last1=Hägele \| first1=Guillermo F.		\| display-authors=1 \| last1=Hägele \| first1=Guillermo F.
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	\| volume=378 \| issue=1 \| pages=163−178 \| date=June 2007		\| volume=378 \| issue=1 \| pages=163−178 \| date=June 2007
	\| doi=10.1111/j.1365-2966.2007.11751.x		\| doi=10.1111/j.1365-2966.2007.11751.x
	\| bibcode=2007MNRAS.378..163H \| arxiv=astro-ph/0703140}}</ref>		\| doi-access=free \| bibcode=2007MNRAS.378..163H \| arxiv=astro-ph/0703140\| s2cid=17402226 }}</ref>

		⚫	A ], designated as SN 2012aw, was discovered in M95 in 2012.{{efn\|On 16 March}}<ref name=DeepSkyVideos>{{cite web
	==Galaxy group information==
		⚫	\| title=Deep Sky Videos
⚫	M95 is one of several galaxies within the ], a ] in the ] ]. ~~The group also includes the~~ ] ] and ].<ref name="nbg">{{cite book
		⚫	\| website=] \| url=https://www.youtube.com/user/DeepSkyVideos?feature=watch
		⚫	\| access-date=19 March 2012
		⚫	}}</ref><ref name=BadAstronomyM95>{{cite web
		⚫	\| title=Supernova 2012aw: the pictures!
		⚫	\| url=http://blogs.discovermagazine.com/badastronomy/2012/03/20/supernova-2012aw-the-pictures/
		⚫	\| access-date=19 March 2012
			\| archive-date=20 October 2019
			\| archive-url=https://web.archive.org/web/20191020161204/http://blogs.discovermagazine.com/badastronomy/2012/03/20/supernova-2012aw-the-pictures/
			\| url-status=dead
		⚫	}}</ref><ref name="IAU Central Bureau for Astronomical Telegrams">{{cite web
		⚫	\| title=List of Recent Supernovae
		⚫	\| url=http://www.cbat.eps.harvard.edu/lists/RecentSupernovae.html
		⚫	\| access-date=8 April 2012
		⚫	}}</ref> The ] of this displayed great flattening after 27 days, thus classifying it as a Type II-P, or "plateau", core-collapse supernova.<ref name=Bayless2013>{{citation
		⚫	\| title=The Long-lived UV "Plateau" of SN 2012aw
		⚫	\| last1=Bayless \| first1=Amanda J. \| last2=Pritchard \| first2=Tyler A.
		⚫	\| last3=Roming \| first3=Peter W. A. \| last4=Kuin \| first4=Paul
		⚫	\| last5=Brown \| first5=Peter J. \| last6=Botticella \| first6=Maria Teresa
		⚫	\| last7=Dall'Ora \| first7=Massimo \| last8=Frey \| first8=Lucille H.
		⚫	\| last9=Even \| first9=Wesley \| last10=Fryer \| first10=Chris L.
		⚫	\| last11=Maund \| first11=Justyn R. \| last12=Fraser \| first12=Morgan
		⚫	\| display-authors=1 \|postscript=.
		⚫	\| journal=The Astrophysical Journal Letters
		⚫	\| volume=764 \| issue=1 \| id=L13 \| pages=6 \| date=February 2013
		⚫	\| doi=10.1088/2041-8205/764/1/L13 \| bibcode=2013ApJ...764L..13B
		⚫	\| arxiv=1210.5496\| s2cid=119291438 }}</ref> The disappearance of the progenitor star was later confirmed from near-infrared imaging of the region. The brightness from the presumed ] progenitor allowed its mass to be estimated as {{Val\|12.5\|1.5\|u=solar mass}}.<ref name=Morgan2016>{{citation
		⚫	\| title=The disappearance of the progenitor of SN 2012aw in late-time imaging
		⚫	\| last1=Fraser \| first1=Morgan \| postscript=.
		⚫	\| journal=Monthly Notices of the Royal Astronomical Society: Letters
		⚫	\| volume=456 \| issue=1 \| pages=L16−L19 \| date=February 2016
		⚫	\| doi=10.1093/mnrasl/slv168 \| doi-access=free \| bibcode=2016MNRAS.456L..16F \| arxiv=1507.06579\| s2cid=118145431 }}</ref>

		⚫	M95 is one of several galaxies within the ], a ] in the ] ], the other ] of which are ] and ].<ref name="nbg">{{cite book
	\| first1=R. B. \| last1=Tully		\| first1=R. B. \| last1=Tully
	\| date=1988 \| title=Nearby Galaxies Catalog		\| date=1988 \| title=Nearby Galaxies Catalog
	\| publisher=]		\| publisher=]
	\| isbn=0-521-35299-1		\| isbn=978-0-521-35299-4
	}}</ref><ref name="fouqueetal1992">{{cite journal		}}</ref><ref name="fouqueetal1992">{{cite journal
	\| first1=P. \| last1=Fouque \| first2=E. \| last2=Gourgoulhon		\| first1=P. \| last1=Fouque \| first2=E. \| last2=Gourgoulhon
Line 87:		Line 121:
	\| date=2000 \| volume=543 \| issue=1 \| pages=178–194		\| date=2000 \| volume=543 \| issue=1 \| pages=178–194
	\| bibcode=2000ApJ...543..178G \| doi=10.1086/317070		\| bibcode=2000ApJ...543..178G \| doi=10.1086/317070
	\| arxiv=astro-ph/0001140 \| display-authors=1		\| arxiv=astro-ph/0001140 \| s2cid=9618325 \| display-authors=1
	}}</ref>		}}</ref>

			]
	==Supernova==
			] and ] instruments.]]
⚫	A ], designated as ], was discovered in M95 on 16 March ~~2012.~~<ref name=DeepSkyVideos>{{cite web

⚫	\| title=Deep Sky Videos
			==See also==
⚫	\| url=https://www.youtube.com/user/DeepSkyVideos?feature=watch
			* ]
⚫	\| ~~accessdate~~=19 March 2012
⚫	}}</ref><ref name=BadAstronomyM95>{{cite web
⚫	\| title=Supernova 2012aw: the pictures!
⚫	\| url=http://blogs.discovermagazine.com/badastronomy/2012/03/20/supernova-2012aw-the-pictures/
⚫	\| ~~accessdate~~=19 March 2012
⚫	}}</ref><ref name="IAU Central Bureau for Astronomical Telegrams">{{cite web
⚫	\| title=List of Recent Supernovae
⚫	\| url=http://www.cbat.eps.harvard.edu/lists/RecentSupernovae.html
⚫	\| ~~accessdate~~=8 April 2012
⚫	}}</ref> The ] of ~~the supernova~~ displayed ~~a significant~~ flattening after 27 days, thus classifying it as a Type II-P, or "plateau", core-collapse supernova.<ref name=Bayless2013>{{citation
⚫	\| title=The Long-lived UV "Plateau" of SN 2012aw
⚫	\| last1=Bayless \| first1=Amanda J. \| last2=Pritchard \| first2=Tyler A.
⚫	\| last3=Roming \| first3=Peter W. A. \| last4=Kuin \| first4=Paul
⚫	\| last5=Brown \| first5=Peter J. \| last6=Botticella \| first6=Maria Teresa
⚫	\| last7=Dall'Ora \| first7=Massimo \| last8=Frey \| first8=Lucille H.
⚫	\| last9=Even \| first9=Wesley \| last10=Fryer \| first10=Chris L.
⚫	\| last11=Maund \| first11=Justyn R. \| last12=Fraser \| first12=Morgan
⚫	\| display-authors=1 \|postscript=.
⚫	\| journal=The Astrophysical Journal Letters
⚫	\| volume=764 \| issue=1 \| id=L13 \| pages=6 \| date=February 2013
⚫	\| doi=10.1088/2041-8205/764/1/L13 \| bibcode=2013ApJ...764L..13B
⚫	\| arxiv=1210.5496}}</ref> The disappearance of the progenitor star was later confirmed from near-infrared imaging of the region. The brightness of the presumed ] progenitor allowed its mass to be estimated as {{Val\|12.5\|1.5\|u=solar mass}}.<ref name=Morgan2016>{{citation
⚫	\| title=The disappearance of the progenitor of SN 2012aw in late-time imaging
⚫	\| last1=Fraser \| first1=Morgan \| postscript=.
⚫	\| journal=Monthly Notices of the Royal Astronomical Society: Letters
⚫	\| volume=456 \| issue=1 \| pages=L16−L19 \| date=February 2016
⚫	\| doi=10.1093/mnrasl/slv168 \| bibcode=2016MNRAS.456L..16F \| arxiv=1507.06579}}</ref>

	==References==		==References==
	{{reflist\|colwidth=30em}}		{{reflist\|colwidth=30em}}
			{{notelist}}

	==External links==		==External links==
			{{commons category}}
	* {{WikiSky}}		* {{WikiSky}}
	*		*
	* {{APOD \|date=14 March 2007 \|title=Barred Spiral Galaxy M95}}		* {{APOD \|date=14 March 2007 \|title=Barred Spiral Galaxy M95}}
	* {{cite web\|last=Merrifield\|first=Michael\|title=Supernova in M95 – SN 2012aw and its progenitor\|url=http://www.deepskyvideos.com/videos/other/supernova_M95_star.html\|work=Deep ~~Space~~ Videos\|publisher=]}}		* {{cite web\|last=Merrifield\|first=Michael\|title=Supernova in M95 – SN 2012aw and its progenitor\|url=http://www.deepskyvideos.com/videos/other/supernova_M95_star.html\|work=Deep Sky Videos\|publisher=]}}

	{{Sky\|10\|43\|57.7\|+\|11\|42\|14\|32600000}}		{{Sky\|10\|43\|57.7\|+\|11\|42\|14\|32600000}}
			{{Portal bar\|Astronomy\|Stars\|Outer space}}

	{{Messier objects}}		{{Messier objects}}

	{{Ngc35}}		{{Ngc35}}

Latest revision as of 03:23, 24 November 2024

Galaxy in the constellation Leo "M95" redirects here. For other uses, see M95 (disambiguation).

Messier 95
Hubble Space Telescope image of Messier 95
Observation data (J2000 epoch)
Constellation	Leo
Right ascension	10 43 57.7
Declination	+11° 42′ 14″
Redshift	778 ± 4 km/s
Distance	32.6 ± 1.4 Mly (10.0 ± 0.4 Mpc)
Apparent magnitude (V)	9.7
Characteristics
Type	SB(r)b
Apparent size (V)	3′.1 × 2′.9
Other designations
NGC 3351, UGC 5850, PGC 32007

Messier 95, also known as M95 or NGC 3351, is a barred spiral galaxy about 33 million light-years away in the zodiac constellation Leo. It was discovered by Pierre Méchain in 1781, and catalogued by compatriot Charles Messier four days later. In 2012 its most recent supernova was discovered.

The galaxy has a morphological classification of SB(r)b, with the SBb notation indicating it is a barred spiral with arms that are intermediate on the scale from tightly to loosely wound, and an "(r)" meaning an inner ring surrounds the bar. The latter is a ring-shaped, circumnuclear star-forming region with a diameter of approximately 70,000 light-years (21,000 pc). The spiral structure extends outward from the ring.

Its ring structure is about 3.5×10 M_☉ (solar masses) in molecular gas and yields a star formation rate of 0.38 M_☉ yr. The star formation is occurring in at least five regions with diameters between 100 and 150 pc that are composed of several star clusters ranging in size from 1.7 to 4.9 pc. These individual clusters contain (1.8–8.7)×10 M_☉ of stars, and may be on the path to forming globular clusters.

A Type II supernova, designated as SN 2012aw, was discovered in M95 in 2012. The light curve of this displayed great flattening after 27 days, thus classifying it as a Type II-P, or "plateau", core-collapse supernova. The disappearance of the progenitor star was later confirmed from near-infrared imaging of the region. The brightness from the presumed red supergiant progenitor allowed its mass to be estimated as 12.5±1.5 M_☉.

M95 is one of several galaxies within the M96 Group, a group of galaxies in the constellation Leo, the other Messier objects of which are M96 and M105.

References

^ "NASA/IPAC Extragalactic Database". Results for NGC 3351. Retrieved 3 October 2007.
Jensen, Joseph B.; Tonry, John L.; Barris, Brian J.; Thompson, Rodger I.; et al. (2003). "Measuring Distances and Probing the Unresolved Stellar Populations of Galaxies Using Infrared Surface Brightness Fluctuations". Astrophysical Journal. 583 (2): 712–726. arXiv:astro-ph/0210129. Bibcode:2003ApJ...583..712J. doi:10.1086/345430. S2CID 551714.
"Messier 95". SEDS Messier Catalog. Retrieved 30 April 2022.
^ Buta, Ronald J.; et al. (2007), Atlas of Galaxies, Cambridge University Press, pp. 1−25, ISBN 978-0521820486.
Colina, L.; Garcia Vargas, M. L.; Mas-Hesse, J. M.; Alberdi, A.; Krabbe, A. (1997). "Nuclear Star-forming Structures and the Starburst–Active Galactic Nucleus Connection in Barred Spirals NGC 3351 and NGC 4303". Astrophysical Journal Letters. 484 (1): L41 – L45. Bibcode:1997ApJ...484L..41C. doi:10.1086/310766.
Hägele, Guillermo F.; et al. (June 2007), "Kinematics of gas and stars in the circumnuclear star-forming ring of NGC3351", Monthly Notices of the Royal Astronomical Society, 378 (1): 163−178, arXiv:astro-ph/0703140, Bibcode:2007MNRAS.378..163H, doi:10.1111/j.1365-2966.2007.11751.x, S2CID 17402226
"Deep Sky Videos". YouTube. Retrieved 19 March 2012.
"Supernova 2012aw: the pictures!". Archived from the original on 20 October 2019. Retrieved 19 March 2012.
"List of Recent Supernovae". Retrieved 8 April 2012.
Bayless, Amanda J.; et al. (February 2013), "The Long-lived UV "Plateau" of SN 2012aw", The Astrophysical Journal Letters, 764 (1): 6, arXiv:1210.5496, Bibcode:2013ApJ...764L..13B, doi:10.1088/2041-8205/764/1/L13, S2CID 119291438, L13.
Fraser, Morgan (February 2016), "The disappearance of the progenitor of SN 2012aw in late-time imaging", Monthly Notices of the Royal Astronomical Society: Letters, 456 (1): L16−L19, arXiv:1507.06579, Bibcode:2016MNRAS.456L..16F, doi:10.1093/mnrasl/slv168, S2CID 118145431.
Tully, R. B. (1988). Nearby Galaxies Catalog. Cambridge University Press. ISBN 978-0-521-35299-4.
Fouque, P.; Gourgoulhon, E.; Chamaraux, P.; Paturel, G. (1992). "Groups of galaxies within 80 Mpc. II – The catalogue of groups and group members". Astronomy and Astrophysics Supplement. 93: 211–233. Bibcode:1992A&AS...93..211F.
Garcia, A. (1993). "General study of group membership. II – Determination of nearby groups". Astronomy and Astrophysics Supplement. 100: 47–90. Bibcode:1993A&AS..100...47G.
Giuricin, G.; et al. (2000). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups". Astrophysical Journal. 543 (1): 178–194. arXiv:astro-ph/0001140. Bibcode:2000ApJ...543..178G. doi:10.1086/317070. S2CID 9618325.
"Caught in the act". eso.org. Retrieved 2 September 2019.

meaning per year
1.8 to 8.7 million solar masses
On 16 March

External links

Messier 95 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
SEDS: Spiral Galaxy M95
NASA Astronomy Picture of the Day: Barred Spiral Galaxy M95 (14 March 2007)
Merrifield, Michael. "Supernova in M95 – SN 2012aw and its progenitor". Deep Sky Videos. Brady Haran.

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v t e New General Catalogue 3000 to 3499
3000 3001 3002 3003 3004 3005 3006 3007 3008 3009 3010 3011 3012 3013 3014 3015 3016 3017 3018 3019 3020 3021 3022 3023 3024 3025 3026 3027 3028 3029 3030 3031 3032 3033 3034 3035 3036 3037 3038 3039 3040 3041 3042 3043 3044 3045 3046 3047 3048 3049 3050 3051 3052 3053 3054 3055 3056 3057 3058 3059 3060 3061 3062 3063 3064 3065 3066 3067 3068 3069 3070 3071 3072 3073 3074 3075 3076 3077 3078 3079 3080 3081 3082 3083 3084 3085 3086 3087 3088 3089 3090 3091 3092 3093 3094 3095 3096 3097 3098 3099 3100 3101 3102 3103 3104 3105 3106 3107 3108 3109 3110 3111 3112 3113 3114 3115 3116 3117 3118 3119 3120 3121 3122 3123 3124 3125 3126 3127 3128 3129 3130 3131 3132 3133 3134 3135 3136 3137 3138 3139 3140 3141 3142 3143 3144 3145 3146 3147 3148 3149 3150 3151 3152 3153 3154 3155 3156 3157 3158 3159 3160 3161 3162 3163 3164 3165 3166 3167 3168 3169 3170 3171 3172 3173 3174 3175 3176 3177 3178 3179 3180 3181 3182 3183 3184 3185 3186 3187 3188 3189 3190 3191 3192 3193 3194 3195 3196 3197 3198 3199 3200 3201 3202 3203 3204 3205 3206 3207 3208 3209 3210 3211 3212 3213 3214 3215 3216 3217 3218 3219 3220 3221 3222 3223 3224 3225 3226 3227 3228 3229 3230 3231 3232 3233 3234 3235 3236 3237 3238 3239 3240 3241 3242 3243 3244 3245 3246 3247 3248 3249 3250 3251 3252 3253 3254 3255 3256 3257 3258 3259 3260 3261 3262 3263 3264 3265 3266 3267 3268 3269 3270 3271 3272 3273 3274 3275 3276 3277 3278 3279 3280 3281 3282 3283 3284 3285 3286 3287 3288 3289 3290 3291 3292 3293 3294 3295 3296 3297 3298 3299 3300 3301 3302 3303 3304 3305 3306 3307 3308 3309 3310 3311 3312 3313 3314 3315 3316 3317 3318 3319 3320 3321 3322 3323 3324 3325 3326 3327 3328 3329 3330 3331 3332 3333 3334 3335 3336 3337 3338 3339 3340 3341 3342 3343 3344 3345 3346 3347 3348 3349 3350 3351 3352 3353 3354 3355 3356 3357 3358 3359 3360 3361 3362 3363 3364 3365 3366 3367 3368 3369 3370 3371 3372 3373 3374 3375 3376 3377 3378 3379 3380 3381 3382 3383 3384 3385 3386 3387 3388 3389 3390 3391 3392 3393 3394 3395 3396 3397 3398 3399 3400 3401 3402 3403 3404 3405 3406 3407 3408 3409 3410 3411 3412 3413 3414 3415 3416 3417 3418 3419 3420 3421 3422 3423 3424 3425 3426 3427 3428 3429 3430 3431 3432 3433 3434 3435 3436 3437 3438 3439 3440 3441 3442 3443 3444 3445 3446 3447 3448 3449 3450 3451 3452 3453 3454 3455 3456 3457 3458 3459 3460 3461 3462 3463 3464 3465 3466 3467 3468 3469 3470 3471 3472 3473 3474 3475 3476 3477 3478 3479 3480 3481 3482 3483 3484 3485 3486 3487 3488 3489 3490 3491 3492 3493 3494 3495 3496 3497 3498 3499
Astronomical catalog List of NGC objects 3001–4000

New General Catalogue 3000 to 3499

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Latest revision as of 03:23, 24 November 2024

See also

References

External links