IC 2448 explained
IC 2448 |
Type: | planetary |
Dist Ly: | 11000 |
Dist Pc: | 3500[1] |
Appmag V: | 11.10[2] |
Names: | Hen 2-19 |
IC 2448 is an elliptical planetary nebula in the constellation of Carina. It was discovered in 1898 by Williamina Fleming.[3] It lies near the bright star Beta Carinae, and the southern Carina can be explored in the months of autumn in the southern hemisphere. The central star of the planetary nebula is an O-type star with a spectral type of O(H)3 III-V.[4] An analysis of Gaia data suggests that it is a binary system.[5]
External links
- http://www.skyfactory.org/deepskycatalogue/IC2448.html
Notes and References
- From parallax, 0.2883 ± 0.0454 mas
- IC 2448. 8 February 2018.
- Web site: New General Catalogue objects: NGC 2440 - 2449. Seligman, Courtney. cseligman.com. 27 September 2019.
- 10.1051/0004-6361/202141916. Planetary nebulae in Gaia EDR3: Central star identification, properties, and binarity. 2021. González-Santamaría. I.. Manteiga. M.. Manchado. A.. Ulla. A.. Dafonte. C.. López Varela. P.. Astronomy & Astrophysics. 656. A51. 2109.12114. 2021A&A...656A..51G. 237940344.
- 10.1051/0004-6361/202140288. Towards a more complete sample of binary central stars of planetary nebulae with Gaia. 2021. Chornay. N.. Walton. N. A.. Jones. D.. Boffin. H. M. J.. Rejkuba. M.. Wesson. R.. Astronomy & Astrophysics. 648. A95. 2101.01800. 2021A&A...648A..95C. 230770301.