NGC 3044
Appearance
NGC 3044 | |
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NGC 3044 is a
major axis aligned along a position angle of 113°.[7] It is a relatively isolated galaxy with no nearby companions.[7] R. B. Tully in 1988 assigned it as a member of the widely displaced Leo Cloud.[3]
The
plane of the sky.[12] The disk appears lob-sided and disturbed, suggesting a recent merger or interaction. There is a diffuse ionized gas extending to 1 kpc above the center of the plane.[7]
The stars in the galaxy have a combined mass of approximately 1.01×1010 M☉,[6] and the star formation rate is 2.77 M☉·yr–1.[6] The total mass of the atomic gas in this galaxy is 3.5×109 M☉,[7] and it has a dust mass of 1.6×108 M☉.[3] The galaxy as a whole has a dynamic mass of 6.4×1010 M☉.[7]
One
References
- ^ S2CID 18913331.
- ^ S2CID 250737862, 50.
- ^ .
- ISBN 9781461406563.
- ^ Bibcode:1995yCat.7026....0N.
- ^ , 58.
- ^ S2CID 119118897, 61.
- ^ "NGC 3044", SIMBAD, Centre de données astronomiques de Strasbourg, retrieved 2023-03-02.
- ^ Erdmann, Jr., Robert E. (December 2006), "NGC Discoverer's List", The NGC/IC Project, retrieved 2023-03-05.
- ^ Seligman, Courtney (Aug 25, 2021), "NGC Objects: NGC 3000 - 3049", Celestial Atlas, retrieved 2023-03-05.
- Bibcode:1973rncn.book.....S.
- Bibcode:1989A&AS...81...51H.
- Bibcode:1988PZ.....22..653T.
- Bibcode:1983IAUC.3787....1A.
- Bibcode:1983IAUC.3789....1K.
- ^ "SN 1983E". Transient Name Server. IAU. Retrieved 5 December 2024.
Further reading
- "NGC 3044", CHANG-E – Continuum Halos in Nearby Galaxies – an ELVA Survey, Queen's University, retrieved 2023-03-04.
- Krause, Marita; et al. (July 2020), "CHANG-ES. XXII. Coherent magnetic fields in the halos of spiral galaxies", Astronomy & Astrophysics, 639, , A112.
- Lee, Siow-Wang; Irwin, Judith A. (November 1997), "Neutral Hydrogen in the Edge-on Spiral Galaxy NGC 3044--Global Properties and Discovery of H I Supershells", The Astrophysical Journal, 490 (1): 247–262, S2CID 14940394.
- Lee, S.; Irwin, J. A. (December 1996), "Neutral hydrogen in the edge-on spiral galaxy NGC 3044: global properties and the discovery of H I supershells.", Journal of the Royal Astronomical Society of Canada, 90: 325, Bibcode:1996JRASC..90R.325L.