NGC 3344
| NGC 3344 | |
|---|---|
 NGC 3344 imaged by the Hubble Space Telescope[1] | |
| Observation data (J2000 epoch) | |
| Constellation | Leo Minor[2] |
| Right ascension | 10h 43m 31.150s[3] |
| Declination | +24° 55′ 19.99″[3] |
| Heliocentric radial velocity | 585[4] km/s |
| Distance | 22.5 Mly (6.9 Mpc)[5] |
| Apparent magnitude (V) | 9.7[2] |
| Characteristics | |
| Type | (R)SAB(r)bc[6] |
| Size | ~84,800 ly (26.01 kpc) (estimated)[7] |
| Apparent size (V) | 7.1′ × 6.5′[2] |
| Other designations | |
| IRAS 10407+2511, UGC 5840, MCG +04-25-046, PGC 31968, CGCG 124-060[7] | |
NGC 3344 is a relatively isolated[8] barred spiral galaxy in the constellation of Leo Minor.[9] It was discovered by German-British astronomer William Herschel on 6 April 1785.[10] This galaxy is located at a distance of 22.5 million light-years (6.9 Mpc)[4] from the Milky Way. It has an apparent visual magnitude of 9.7 and spans an angular size of 7.1′ × 6.5′.[2] The nearest bright galaxy is NGC 3274 at a projected separation of 3.7°.[8] NGC 3344 belongs to the galaxy group known as the Leo spur, which is a branch of the Virgo Supercluster.[11]
The morphological classification of NGC 3344 is (R)SAB(r)bc,[6] which indicates it is a barred spiral galaxy (SAB) that exhibits rings (R, r) and moderate to loosely wound spiral arms (bc).[12] The plane of the galaxy is inclined at an angle of around 25.5° with the long angle of the resulting elliptical shape aligned along a position angle of −23.9°.[8] There is both an inner ring and outer pseudo-ring, with the prominent arms radiating outward from the inner ring and the relatively small and slightly elliptical bar being situated inside. At the center of the bar is an H II nucleus with an angular diameter of about 3″.[8]
Supernova
[edit]One supernova has been observed in NGC 3344: SN 2012fh, a Type Ib/Ic that peaked at magnitude 15.1. It was discovered by Masaki Tsuboi on 18 October 2012.[13][14][15]
References
[edit]- ↑ "A Lonely Beauty". www.spacetelescope.org. 14 February 2018. Retrieved 16 February 2018.
- 1 2 3 4 Finlay, Warren H. (2014), Concise Catalogue of Deep-Sky Objects, The Patrick Moore Practical Astronomy Series (2nd ed.), Springer Cham, p. 246, doi:10.1007/978-3-319-03170-5, ISBN 978-3-319-03169-9.
- 1 2 Skrutskie, Michael F.; et al. (February 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.
- 1 2 Crook, Aidan C.; et al. (February 2007), "Groups of Galaxies in the Two Micron All Sky Redshift Survey", The Astrophysical Journal, 655 (2): 790–813, arXiv:astro-ph/0610732, Bibcode:2007ApJ...655..790C, doi:10.1086/510201, S2CID 11672751.
- ↑ Epinat, B.; et al. (August 2008), "GHASP: an Hα kinematic survey of spiral and irregular galaxies - VI. New Hα data cubes for 108 galaxies", Monthly Notices of the Royal Astronomical Society, 388 (2): 500–550, arXiv:0805.0976, Bibcode:2008MNRAS.388..500E, doi:10.1111/j.1365-2966.2008.13422.x, S2CID 14282151.
- 1 2 Pilyugin, L. S.; et al. (October 2004), "Oxygen and nitrogen abundances in nearby galaxies. Correlations between oxygen abundance and macroscopic properties", Astronomy and Astrophysics, 425 (3): 849–869, arXiv:astro-ph/0407014, Bibcode:2004A&A...425..849P, doi:10.1051/0004-6361:20034522, S2CID 119074817.
- 1 2 "Results for object NGC 3344", NASA/IPAC Extragalactic Database, NASA and Caltech, retrieved 15 May 2007.
- 1 2 3 4 Verdes-Montenegro, L.; et al. (April 2000), "A detailed study of the ringed galaxy NGC 3344", Astronomy and Astrophysics: 827–839, Bibcode:2000A&A...356..827V.
- ↑ "Hubble Sees Galaxy in a spin - NASA Science", science.nasa.gov, 18 October 2012, retrieved 11 November 2024.
- ↑ Seligman, Courtney, "New General Catalogue Objects: NGC 3344", Celestial Atlas, retrieved 8 June 2025.
- ↑ Monks, Neale (2010), Go-to Telescopes Under Suburban Skies, Patrick Moore's Practical Astronomy Series, Springer, p. 53, ISBN 978-1441968517.
- ↑ Buta, Ronald J.; et al. (2007), Atlas of Galaxies, Cambridge University Press, pp. 13–17, ISBN 978-0521820486.
- ↑ Nakano, S.; et al. (2012), "Supernova 2012fh in NGC 3344 = PSN J10433405+2453290", Central Bureau Electronic Telegrams (3263): 1, Bibcode:2012CBET.3263....1N.
- ↑ Johnson, Samson A.; et al. (April 2013), "On the progenitor of the Type Ibc supernova 2012fh", Monthly Notices of the Royal Astronomical Society, 472 (3): 3115–3119, arXiv:1707.03828, Bibcode:2017MNRAS.472.3115J, doi:10.1093/mnras/stx2170.
- ↑ "SN 2012fh", Transient Name Server, IAU, retrieved 8 June 2025.
Further reading
[edit]- Padave, Mansi; et al. (December 2021), "DIISC-II: Unveiling the Connections between Star Formation and Interstellar Medium in the Extended Ultraviolet Disk of NGC 3344", The Astrophysical Journal, 923 (2), id. 199, arXiv:2110.07590, Bibcode:2021ApJ...923..199P, doi:10.3847/1538-4357/ac2c01.
- Akyuz, Aysun (2010), "New SNR candidates in nearby spiral galaxy NGC 3344", 38th COSPAR Scientific Assembly. Held 18-15 July 2010, in Bremen, Germany, id. 2813, Bibcode:2010cosp...38.2813A.
- Moumen, Ismael; et al. (June 2019), "3D Optical Spectroscopic Study of NGC 3344 with SITELLE: I. Identification and Confirmation of Supernova Remnants", Supernova Remnants: An Odyssey in Space after Stellar Death II, held 3-8 June 2019 in Chania, Greece, id. 54, Bibcode:2019sros.confE..54M.
- Corbelli, Edvige; et al. (February 1989), "H I Mapping of Outer Disks of Galaxies. M33 and NGC 3344", Astronomical Journal, 97: 390, Bibcode:1989AJ.....97..390C, doi:10.1086/114989.
- Vilchez, J. M.; et al. (November 1988), "The Abundance Gradient in NGC 3344", Publications of the Astronomical Society of the Pacific, Bibcode:1988PASP..100.1428V, doi:10.1086/132343.
- McCall, M. L.; et al. (June–July 1981), "NGC 3344 - Unusual abundances for an SBC galaxy", Astronomical Society of the Pacific, Publications, 93: 273–278, Bibcode:1981PASP...93..273M, doi:10.1086/130821.
External links
[edit]
Media related to NGC 3344 at Wikimedia Commons- Galex image of NGC 3344
