IC 1295是位於盾牌座的行星狀星雲,距離地球大約4,700光年(1,500秒差距)[2]。杜魯門·薩福德(Truman Safford)於1867年發現IC 1295[4]。
行星狀星雲的中心恆星的光譜類型為DAO.56,顯示缺氫類天體為hgO(H)[5]。
參考資料
- ^ 1.0 1.1
SIMBAD Astronomical Database. Results for IC 1295. [2011-06-02].
- ^ 2.0 2.1 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.
- ^ 3.0 3.1
NGC/IC Project. Results for IC 1295. [2011-06-02]. (原始内容存档于2012-05-20).
- ^ Seligman, Courtney. New General Catalogue objects: NGC 1250 - 1299. cseligman.com. [27 September 2019].
- ^ González-Santamaría, I.; Manteiga, M.; Manchado, A.; Ulla, A.; Dafonte, C.; López Varela, P. Planetary nebulae in Gaia EDR3: Central star identification, properties, and binarity. Astronomy & Astrophysics. 2021, 656: A51. Bibcode:2021A&A...656A..51G. S2CID 237940344. arXiv:2109.12114 . doi:10.1051/0004-6361/202141916.
外部連結