NGC 3432
NGC 3432 is an edge-on spiral galaxy that can be found in the northern constellation of Leo Minor. It was discovered by German-British astronomer William Herschel on March 19, 1787. This galaxy is located at a distance of 40 million light-years (12.3 Mpc) from the Milky Way. It is interacting with UGC 5983, a nearby dwarf galaxy, and features tidal filaments and intense star formation. Because of these features, it was listed in Halton Arp's Atlas of Peculiar Galaxies.
Hubble image of NGC 3432 showing regions of
star formation
The morphological classification of NGC 3432 is SB(s)m, which indicates this is a barred Magellanic spiral galaxy (SB) with no inner ring structure (s) and an irregular appearance (m). The galaxy is inclined at an angle of 85°±2° to the plane of the sky with its major axis along a positional angle of 38°, which means it is being viewed from nearly edge-on. It is interacting with the companion galaxy UGC 5983, which is creating features that extend outside the galactic plane, as well as an extended halo of radio emission. The shape of the galaxy is distorted and two tidal tails have been identified. NGC 3432 has an active galactic nucleus of the LINER type with a nuclear HII region.
In May 3, 2000, a candidate nova was detected in this galaxy. It was located 123″ east and 180″ north of the galactic nucleus, and aligned with an H II region (or spiral arm) of the galaxy. This appeared similar to a type IIn supernova (designated SN 2000ch), but it peaked below the typical luminosity of these events. As such, it may have been a "superoutburst" of a luminous variable and thus it could have survived the event. The outburst was found comparable to an eruption of Eta Carinae in the mid–nineteenth century. Multiple subsequent outbursts were observed in 2008 and 2009. It is now classified as a supernova imposter, and is expected to become a core collapse supernova in the future.
References
- ^ 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 Kourkchi, Ehsan; et al. (October 23, 2020), "Cosmicflows-4: The Catalog of ∼10,000 Tully–Fisher Distances", The Astrophysical Journal, 902 (2): 145, arXiv:2009.00733, Bibcode:2020ApJ...902..145K, doi:10.3847/1538-4357/abb66b, ISSN 1538-4357.
- ^ a b Gilmour, Jess K. (2003), The Practical Astronomer’s Deep-sky Companion, Springer London, p. 73, ISBN 1-85233-474-6.
- ^ a b c English, Jayanne; Irwin, Judith A. (June 1997), "The Ionized Gas and Radio Halo of NGC 3432 (ARP 206)", Astronomical Journal, 113: 2006–2024, Bibcode:1997AJ....113.2006E, doi:10.1086/118413.
- ^ "NGC 3432". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2024-03-15.
- ^ "Feeling Edgy". www.spacetelescope.org. Retrieved 29 July 2019.
- ^ Seligman, Courtney. "Celestial Atlas NGC Objects 2850-2899". Celestial Atlas. Retrieved 2024-03-15.
- ^ Arp, Halton (1966). Atlas of Peculiar Galaxies. Pasadena, California: California Institute of Technology. Retrieved 5 Jan 2010.
- ^ Hubble Traces a Galaxy’s Outer Reaches, NASA Hubble Mission Team, Goddard Spaceflight Center, August 2, 2019, retrieved 2024-03-16.
- ^ Irwin, Judith A.; et al. (April 2000), "High-Resolution Radio Continuum Observations of Edge-on Spiral Galaxies", The Astronomical Journal, 119 (4): 1592–1607, Bibcode:2000AJ....119.1592I, doi:10.1086/301287.
- ^ Wagner, R. M.; et al. (May 2000), Green, D. W. E. (ed.), "Variable Star in NGC 3432", IAU Circular, 7417: 2, Bibcode:2000IAUC.7417....2W.
- ^ Papenkova, M.; Li, W. D. (May 2000), Green, D. W. E. (ed.), "Variable Star in Field of NGC 3432", IAU Circular, 7415: 1, Bibcode:2000IAUC.7415....1P.
- ^ Filippenko, A. V. (May 2000), Green, D. W. E. (ed.), "Supernova 2000ch in NGC 3432", IAU Circular, 7421: 3, Bibcode:2000IAUC.7421....3F.
- ^ Wagner, R. M.; et al. (April 2004), "Discovery and Evolution of an Unusual Luminous Variable Star in NGC 3432 (Supernova 2000ch)", The Publications of the Astronomical Society of the Pacific, 116 (818): 326–336, arXiv:astro-ph/0404035, Bibcode:2004PASP..116..326W, doi:10.1086/382997.
- ^ Pastorello, A.; et al. (October 2010), "Multiple major outbursts from a restless luminous blue variable in NGC 3432", Monthly Notices of the Royal Astronomical Society, 408 (1): 181–198, arXiv:1006.0504, Bibcode:2010MNRAS.408..181P, doi:10.1111/j.1365-2966.2010.17142.x.
- ^ Müller, Ancla; et al. (February 2023), "Multi-epoch variability of AT 2000ch (SN 2000ch) in NGC 3432. A radio continuum and optical study", Astronomy & Astrophysics, 670, id. A130, arXiv:2211.15706, Bibcode:2023A&A...670A.130M, doi:10.1051/0004-6361/202142139.
External links
- Bertola, F. (1966), "Mass and luminosity distribution in galaxies NGC 3432, NGC 4485-90 and NGC 4605.", Memorie della Societa Astronomica Italiana, 37: 433–458, Bibcode:1966MmSAI..37..433B.
- "NASA/IPAC Extragalactic Database", Results for NGC 3432, retrieved 2008-04-10.
Media related to NGC 3432 at Wikimedia Commons- NGC 3432 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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SDSS DR14 image of NGC 3432
Hubble image of NGC 3432 showing regions of star formation
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