NGC 4245是一个位于后发座的透鏡狀星系[3]，1785年3月13日由威廉·赫歇爾发现[5]，属于后发座I星系群[6]。
- ^ 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. VizieR中此天体在盖亚望远镜第二批数据发布的记录
- ^ 2.0 2.1 2.2 2.3 NGC 4245. SIMBAD. 斯特拉斯堡天文資料中心. [2021-05-28].
- ^ 3.0 3.1 3.2 Marino, Antonietta; Bianchi, Luciana; Rampazzo, Roberto; Thilker, David A.; Annibali, Francesca; Bressan, Alessandro; Buson, Lucio Maria. Tracing Rejuvenation Events in Nearby S0 Galaxies. The Astrophysical Journal. 2011, 736 (2): 154. Bibcode:2011ApJ...736..154M. arXiv:1105.3812 . doi:10.1088/0004-637X/736/2/154.
- ^ 4.0 4.1 Search specification: NGC 4245. HyperLeda. Université Claude Bernard Lyon 1. [2021-05-28]. （原始内容存档于2022-07-05）.
- ^ Seligman, Courtney. New General Catalogue objects: NGC 4200 - 4249. cseligman.com. [2021-05-28]. （原始内容存档于2019-02-09）.
- ^ Sil'chenko, O. K.; Chilingarian, I. V.; Afanasiev, V. L. NGC 4245: one or two bars, and where does the gas inflow stop?.. Memorie della Societa Astronomica Italiana Supplementi. 2011-01-01, 18: 159 [2022-07-05]. ISSN 0037-8720. （原始内容存档于2022-01-23）.
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