梅西耶星表/M84

梅西耶 84
梅西耶 84
	200px M84。来源：w:NOAO.
观测数据 (w:J2000 历元)
星座	室女座
赤经	12h 25m 03.7s
赤纬	+12° 53′ 13″
红移	1060 ± 6 km/s
距离	60 ± 3 百万光年 (18.4 ± 0.9 Mpc)
类型	E1
视尺寸 (V)	6′.5 × 5′.6
视星等 (V)	10.1
显著特征	-
其他名称
	NGC 4374, UGC 7494, PGC 40455, VCC 763

梅西耶84（也称为M84或NGC 4374）是室女座的一个w:透镜状星系。M84位于室女座星系团人口稠密的核心区域。^[3]

无线电观测和w:哈勃太空望远镜对M84的图像揭示了从星系中心射出的两股物质喷流，以及靠近星核的快速旋转的气体和恒星盘，表明该星系核心中存在着一个质量为18 ×10⁸ M_☉^[4]的超大质量w:黑洞。

历史

w:查尔斯·梅西耶于1781年3月18日在夜空中系统地寻找“星云状天体”时发现了梅西耶84^[5]。该天体在w:梅西耶星表中排名第84位。

超新星

在M84中已观测到两颗w:超新星：w:SN 1957^[6]和w:SN 1991bg.^[7] 可能，第三颗w:SN 1980I是M84的一部分，或者，它可能属于其邻近星系之一，w:NGC 4387和M86.^[8]

外部链接

SEDS 透镜状星系 M84

参考文献

↑ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^j "NASA/IPAC Extragalactic Database". Results for NGC 4374. Retrieved 2006-11-14.
↑ J. L. Tonry, A. Dressler, J. P. Blakeslee, E. A. Ajhar, A. B. Fletcher, G. A. Luppino, M. R. Metzger, C. B. Moore (2001). "The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances". Astrophysical Journal. 546 (2): 681–693. doi:10.1086/318301.{{cite journal}}: CS1 maint: multiple names: authors list (link)
↑ Finoguenov, A.; Jones, C. (2002). "Chandra Observation of Low-Mass X-Ray Binaries in the Elliptical Galaxy M84". The Astrophysical Journal. 574 (2): 754–761. doi:10.1086/340997.{{cite journal}}: CS1 maint: multiple names: authors list (link)
↑ Ly, C.; Walker, R. C.; Wrobel, J. M. (2004). "An Attempt to Probe the Radio Jet Collimation Regions in NGC 4278, NGC 4374 (M84), and NGC 6166". The Astronomical Journal. 127 (1): 119–124. doi:10.1086/379855.{{cite journal}}: CS1 maint: multiple names: authors list (link)
↑ K. G. Jones (1991). Messier's Nebulae and Star Clusters (2nd ed.). Cambridge: Cambridge University Press. ISBN 0-521-37079-5.
↑ Götz, W. (1958). "Supernova in NGC 4374 (= M 84)". Astronomische Nachrichten. 284: 141. doi:10.1002/asna.19572840308.
↑ Kosai, H.; Kushida, R.; Kato, T.; Filippenko, A.; Newberg, H. (1958). "超新星1991bg在NGC 4374中的位置". IAU Circ. 5400: 1.{{cite journal}}: CS1 maint: multiple names: authors list (link)
↑ Smith, H. A. (1981). "星际超新星1980I的光谱". Astronomical Journal. 86: 998–1002. doi:10.1086/112975. {{cite journal}}: Unknown parameter |month= ignored (help)

[ned-1] ↑ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^j "NASA/IPAC Extragalactic Database". Results for NGC 4374. Retrieved 2006-11-14.

[tonryetal2001-2] J. L. Tonry, A. Dressler, J. P. Blakeslee, E. A. Ajhar, A. B. Fletcher, G. A. Luppino, M. R. Metzger, C. B. Moore (2001). "The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances". Astrophysical Journal. 546 (2): 681–693. doi:10.1086/318301.{{cite journal}}: CS1 maint: multiple names: authors list (link)

[Finoguenovetal2002-3] Finoguenov, A.; Jones, C. (2002). "Chandra Observation of Low-Mass X-Ray Binaries in the Elliptical Galaxy M84". The Astrophysical Journal. 574 (2): 754–761. doi:10.1086/340997.{{cite journal}}: CS1 maint: multiple names: authors list (link)

[Lyetal2004-4] Ly, C.; Walker, R. C.; Wrobel, J. M. (2004). "An Attempt to Probe the Radio Jet Collimation Regions in NGC 4278, NGC 4374 (M84), and NGC 6166". The Astronomical Journal. 127 (1): 119–124. doi:10.1086/379855.{{cite journal}}: CS1 maint: multiple names: authors list (link)

[jonesbook1991-5] K. G. Jones (1991). Messier's Nebulae and Star Clusters (2nd ed.). Cambridge: Cambridge University Press. ISBN 0-521-37079-5.

[Götz1958-6] Götz, W. (1958). "Supernova in NGC 4374 (= M 84)". Astronomische Nachrichten. 284: 141. doi:10.1002/asna.19572840308.

[Kosaietal1991-7] Kosai, H.; Kushida, R.; Kato, T.; Filippenko, A.; Newberg, H. (1958). "超新星1991bg在NGC 4374中的位置". IAU Circ. 5400: 1.{{cite journal}}: CS1 maint: multiple names: authors list (link)

[Smith1981-8] Smith, H. A. (1981). "星际超新星1980I的光谱". Astronomical Journal. 86: 998–1002. doi:10.1086/112975. {{cite journal}}: Unknown parameter |month= ignored (help)

[1]

[2]

[3]

[4]

[5]

[6]

[7]

[8]