NGC 709 - 维基百科，自由的百科全书

NGC 709 是一个位于仙女座的透镜状星系，距离地球1.5亿光年 。^[1] 由爱尔兰工程师和天文学家Bindon Blood Stoney于1850年10月28日发现，^[2] 是星系团Abell 262的成员。^{[3][4][5][6][7][8]}

维基共享资源上的相關多媒體資源：NGC 709

• NED – NGC 709
• SEDS – NGC 709
• SIMBAD – NGC 709
• VizieR – NGC 709

1. ^ Your NED Search Results. ned.ipac.caltech.edu. [2018-12-27]. （原始内容存档于2022-02-16）. 
2. ^ New General Catalog Objects: NGC 700 - 749. cseligman.com. [2018-11-21]. （原始内容存档于2019-03-22） （美国英语）. 
3. ^ NGC 709. sim-id. [2018-12-27]. （原始内容存档于2022-02-16）. 
4. ^ Steinicke, Wolfgang. Observing and Cataloguing Nebulae and Star Clusters: From Herschel to Dreyer's New General Catalogue. Cambridge University Press. 2010-08-19: 309 [2022-02-16]. ISBN 978-1-139-49010-8. （原始内容存档于2022-02-16）. 
5. ^ Scodeggio, Marco; Boselli, Alessandro; Gavazzi, Giuseppe; Trinchieri, Ginevra; Garilli, Bianca. Multifrequency windows on spiral galaxies. II - The A262 and Cancer clusters. Astronomy and Astrophysics Supplement Series. 1992-08-01, 94: 299–326. Bibcode:1992A&AS...94..299S. ISSN 0365-0138. 
6. ^ Butcher, H. R.; Oemler, A. Jr. The evolution of galaxies in clusters. IV - Photometry of 10 low-redshift clusters. The Astrophysical Journal Supplement Series. 1985-04-01, 57: 665–691. Bibcode:1985ApJS...57..665B. ISSN 0067-0049. doi:10.1086/191022. 
7. ^ Fanti, C.; Fanti, R.; Feretti, L.; Ficarra, A.; Gioia, I. M.; Giovannini, G.; Gregorini, L.; Mantovani, F.; Marano, B. Radio and optical observations of 9 nearby Abell clusters - A262, A347, A569, A576, A779, A1213, A1228, A2162, A2666. Astronomy and Astrophysics. 1982-01-01, 105: 200–218. Bibcode:1982A&A...105..200F. ISSN 0004-6361. 
8. ^ Moss, C.; Dickens, R. J. Redshifts of galaxies in the cluster Abell 262, and in the region of the Pisces group /centred on NGC 383/. Monthly Notices of the Royal Astronomical Society. 1977-03-01, 178 (4): 701–715. Bibcode:1977MNRAS.178..701M. ISSN 0035-8711. doi:10.1093/mnras/178.4.701 . 

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