NGC 66

NGC 66
	Pan-STARRS image of NGC 66
观测资料（J2000 历元）
星座	Cetus
赤经	00h 19m 04.94039s
赤纬	-22° 56′ 10.8306″
红移	0.025368
径向速度	7509 km/s
距离	286.69 ± 0.65 Mly（87.90 ± 0.20 Mpc）
视星等 (B)	14.21
特征
类型	SB(r)b pec
其他名称
	MCG-04-02-002、PGC 1236
	参见：星系、星系列表

NGC 66是鲸鱼座的一个漩涡星系。星等为13.4，赤经为19分04.9秒，赤纬为-22°56'11"。1886年由法兰克·穆勒首次发现^[5]，含有广大的电离氢区^[6]。此星系离地球较远，估算其大小时，需要考虑宇宙的膨胀幅度，估算值达130000光年。^[5]此星系中心之外，有某个无线电波源^[7]，旋臂上亦有红外线源^[8]。

参见[编辑]

NGC天体列表

参考文献[编辑]

^ ^1.0 ^1.1 Brown, A. G. A.; Vallenari, A.; Prusti, T.; de Bruijne, J. H. J.; et al. Gaia Data Release 2. Summary of the contents and survey properties. Astronomy & Astrophysics. 2018. Bibcode:2018A&A...616A...1G. arXiv:1804.09365 . doi:10.1051/0004-6361/201833051.
^ ^2.0 ^2.1 ^2.2 ^2.3 NGC 66. SIMBAD. 斯特拉斯堡天文资料中心. [2021-02-13].
^ Tully, R. Brent; et al. Cosmicflows-2: The Data. The Astronomical Journal. 2013, 146 (4): 86. Bibcode:2013AJ....146...86T. S2CID 118494842. arXiv:1307.7213 . doi:10.1088/0004-6256/146/4/86.
^ Results for object NGC 0066 (NGC 66). NASA/IPAC Extragalactic Database. California Institute of Technology. [2021-02-13]. （原始内容存档于2022-05-07）.
^ ^5.0 ^5.1 Seligman, Countney. Celestial Atlas, NGC Objects: NGC 50 - 99. [2022-03-06]. （原始内容存档于2018-10-24）.
^ NASA/IPAC Extragalactic Database. 2016-01-13 （英语）.
^ Unger, S. W.; Wolstencroft, R. D.; Pedlar, A.; Savage, A.; Clowes, R. G. The relationship between the radio and far-infrared emission in IRAS galaxies: VLA observations of a large well-defined sample at 1420 MHz. Monthly Notices of the Royal Astronomical Society (Oxford University Press). 1989-2, 236 (3): 425—446. ISSN 0035-8711. doi:10.1093/mnras/236.3.425 （英语）. 请检查|date=中的日期值 (帮助)
^ Wolstencroft, R. D.; Savage, A.; Clowes, R. G.; MacGillivray, H. T.; Leggett, S. K. The identification of IRAS point sources – I. A 304 deg2 field centred on the South Galactic Pole. Monthly Notices of the Royal Astronomical Society (Oxford University Press). 1986-11, 223 (2): 279—302. ISSN 0035-8711. doi:10.1093/mnras/223.2.279 （英语）.

天文学目录
NGC天体表：	NGC 64 - NGC 65 - NGC 66 - NGC 67 - NGC 68

这是一篇与星系相关的小作品。你可以通过编辑或修订扩充其内容。

[GaiaDR2-1] 1.0 ^1.1 Brown, A. G. A.; Vallenari, A.; Prusti, T.; de Bruijne, J. H. J.; et al. Gaia Data Release 2. Summary of the contents and survey properties. Astronomy & Astrophysics. 2018. Bibcode:2018A&A...616A...1G. arXiv:1804.09365 . doi:10.1051/0004-6361/201833051.

[SIMBAD-2] 2.0 ^2.1 ^2.2 ^2.3 NGC 66. SIMBAD. 斯特拉斯堡天文资料中心. [2021-02-13].

[Cosmicflows2-3] Tully, R. Brent; et al. Cosmicflows-2: The Data. The Astronomical Journal. 2013, 146 (4): 86. Bibcode:2013AJ....146...86T. S2CID 118494842. arXiv:1307.7213 . doi:10.1088/0004-6256/146/4/86.

[NED-4] Results for object NGC 0066 (NGC 66). NASA/IPAC Extragalactic Database. California Institute of Technology. [2021-02-13]. （原始内容存档于2022-05-07）.

[:0-5] 5.0 ^5.1 Seligman, Countney. Celestial Atlas, NGC Objects: NGC 50 - 99. [2022-03-06]. （原始内容存档于2018-10-24）.

[ned-6] NASA/IPAC Extragalactic Database. 2016-01-13 （英语）.

[7] Unger, S. W.; Wolstencroft, R. D.; Pedlar, A.; Savage, A.; Clowes, R. G. The relationship between the radio and far-infrared emission in IRAS galaxies: VLA observations of a large well-defined sample at 1420 MHz. Monthly Notices of the Royal Astronomical Society (Oxford University Press). 1989-2, 236 (3): 425—446. ISSN 0035-8711. doi:10.1093/mnras/236.3.425 （英语）. 请检查|date=中的日期值 (帮助)

[8] Wolstencroft, R. D.; Savage, A.; Clowes, R. G.; MacGillivray, H. T.; Leggett, S. K. The identification of IRAS point sources – I. A 304 deg2 field centred on the South Galactic Pole. Monthly Notices of the Royal Astronomical Society (Oxford University Press). 1986-11, 223 (2): 279—302. ISSN 0035-8711. doi:10.1093/mnras/223.2.279 （英语）.

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