NGC 3044
| NGC 3044 | |
|---|---|
 legacy surveys image of NGC 3044 | |
| Observation data (J2000 epoch) | |
| Constellation | Sextans |
| Right ascension | 09h 53m 40.884s[1] |
| Declination | +01° 34′ 46.74″[1] |
| Heliocentric radial velocity | 1,289 km/s[2] |
| Galactocentric velocity | 1,130 km/s[2] |
| Distance | 67 Mly (20.6 Mpc)[2] |
| Group or cluster | Leo Cloud[3] |
| Apparent magnitude (V) | 12.5[4] |
| Apparent magnitude (B) | 12.4[5] |
| Characteristics | |
| Type | SBc[6] |
| Mass | 6.4×1010[7] M☉ |
| Notable features | Edge-on galaxy |
| Other designations | |
| IRAS 09511+0148, 2MASX J09534088+0134467, UGC 5311, LEDA 28517, MCG +00-25-031, PGC 28517, CGCG 007-056[8] | |
NGC 3044 is a barred spiral galaxy in the equatorial constellation of Sextans. It was discovered on December 13, 1784, by German-born English astronomer William Herschel.[9][10] In 1888, Danish astronomer J. L. E. Dreyer described it as "very faint, very large, very much extended 122°".[11] It is located at an estimated distance of 67 million light years.[2] In the B band of the UBV photometric system, the galaxy spans 4.70′ by 0.80′[5] with the 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 morphological classification of NGC 3044 is SBc,[6] indicating a barred spiral (SB) with somewhat loosely-wound spiral arms (c). It is being viewed edge-on, with a galactic plane that is inclined at an angle of 79°±4° to 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 supernova has been observed in NGC 3044: SN 1983E (type II, mag. 14)[13] was discovered by Natalʹja Metlova on 13 March 1983, at an offset 29″ east, 11″ south of the galaxy.[14][15][16]
References
[edit]- ^ a b Skrutskie, Michael F.; et al. (February 1, 2006), "The Two Micron All Sky Survey (2MASS)", The Astronomical Journal, 131 (2): 1163–1183, Bibcode:2006AJ....131.1163S, doi:10.1086/498708, ISSN 0004-6256, S2CID 18913331.
- ^ a b c d Tully, R. Brent; et al. (August 2016), "Cosmicflows-3", The Astronomical Journal, 152 (2): 21, arXiv:1605.01765, Bibcode:2016AJ....152...50T, doi:10.3847/0004-6256/152/2/50, S2CID 250737862, 50.
- ^ a b c Irwin, J. A.; et al. (August 2013), "The 617 MHz-λ 850 μm correlation (cosmic rays and cold dust) in NGC 3044 and NGC 4157", Monthly Notices of the Royal Astronomical Society, 433 (4): 2958–2974, arXiv:1306.0226, Bibcode:2013MNRAS.433.2958I, doi:10.1093/mnras/stt937.
- ^ Cavin, Jerry D. (2011), The Amateur Astronomer's Guide to the Deep-Sky Catalogs, Springer New York, p. 167, ISBN 9781461406563.
- ^ a b Nilson, Peter (1973), "Uppsala general catalogue of galaxies", VizieR On-line Data Catalog: VII/26D, Bibcode:1995yCat.7026....0N.
- ^ a b c d Hodges-Kluck, Edmund; et al. (December 2016), "Ultraviolet Halos around Spiral Galaxies. I. Morphology", The Astrophysical Journal, 833 (1): 58, arXiv:1610.02404, Bibcode:2016ApJ...833...58H, doi:10.3847/1538-4357/833/1/58, 58.
- ^ a b c d e f Zschaechner, Laura K.; et al. (January 2015), "Investigating Disk-halo Flows and Accretion: A Kinematic and Morphological Analysis of Extraplanar H I in NGC 3044 and NGC 4302", The Astrophysical Journal, 799 (1): 61, arXiv:1411.2593, Bibcode:2015ApJ...799...61Z, doi:10.1088/0004-637X/799/1/61, 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.
- ^ Sulentic, Jack W.; et al. (1973), The Revised New Catalogue of Nonstellar Astronomical Objects, Tucson: University of Arizona Press, Bibcode:1973rncn.book.....S.
- ^ Singal, J.; et al. (November 1989), "Axial Ratio of Edge-On Spiral Galaxies as a Test for Bright Radio Halos", Astronomy and Astrophysics Supplement Series, 81: 51–58, Bibcode:1989A&AS...81...51H.
- ^ Tsvetkov, D. Yu. (1988). "Light curves of five supernovae". Peremennye Zvezdy. 22: 653. Bibcode:1988PZ.....22..653T.
- ^ Aksenov, E. P.; Terebizh, Yu. V.; Maza, J.; Gonzalez, L. E. (1983). "Supernovae". International Astronomical Union Circular (3787): 1. Bibcode:1983IAUC.3787....1A.
- ^ Kosai, H.; et al. (April 1983), Marsden, B. G. (ed.), "Supernovae", IAU Circular, 3789 (1), Bibcode:1983IAUC.3789....1K.
- ^ "SN 1983E". Transient Name Server. IAU. Retrieved 5 December 2024.
Further reading
[edit]- "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, arXiv:2004.14383, Bibcode:2020A&A...639A.112K, doi:10.1051/0004-6361/202037780, 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, arXiv:astro-ph/9710182, Bibcode:1997ApJ...490..247L, doi:10.1086/304840, 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.
