Astronomy:NGC 157

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Short description: Galaxy in the constellation Cetus
NGC 157
NGC 157.jpg
VLT image of NGC 157
Observation data (J2000 epoch)
ConstellationCetus
Right ascension 00h 34m 46.751s[1]
Declination−08° 23′ 47.36″[1]
Redshift0.0055[2]
Helio radial velocity1651 km/s[3]
Distance39.4 Mly (12.1 Mpc)[3]
75 Mly (23 Mpc)[4]
Apparent magnitude (V)10.4[5]
Apparent magnitude (B)11.07[3]
Characteristics
TypeSAB(rs)bc[6]
Size90 kly[7]
Apparent size (V)4.0′ × 2.4′[5]
Other designations
MCG-02-02-056, PGC 2081, 2MASSX J00344675-0823473[2]

NGC 157 is an intermediate spiral galaxy in the constellation of Cetus, positioned about 4° east of the star Iota Ceti. This galaxy can be viewed from suburban skies using a moderate-sized telescope.[5] It was discovered on December 13, 1783 by William Herschel. The compiler of the New General Catalogue, John Louis Emil Dreyer noted that NGC 157 was "pretty bright, large, extended, between 2 considerably bright stars".[7] It is a relatively isolated galaxy; the nearest other galaxy of comparable luminosity lies at a separation of 4.2 Mly (1.3 Mpc).[8]

NGC 157 from the Mount Lemmon SkyCenter using the 0.8m Schulman Telescope

The morphological classification of NGC 157 is SAB(rs)bc,[6] indicating this is a weakly-barred spiral galaxy (SAB) with a transitional ring structure (rs) and moderate to loosely-wound arms (bc). The plane of the galaxy is inclined at an angle of 61.8° to the line of sight from the Earth.[6] It has symmetric arms that become flocculent in the outer parts, breaking into multiple arms. The rotation curve for this galaxy undergoes a sharp decline, suggesting a low mass or a small dark matter halo.[8] It is considered a quiescent galaxy, showing little star formation activity.[9] However, there is a starburst region in the nucleus forming new stars at the rate of about one solar mass per year.[10]

This galaxy has been host to two observed supernova events. The first, 2009em, was discovered 5 May 2009, about 34″ west and 10″ south of the galaxy core.[11] It was determined to be a Type Ic supernova.[12] On 5 May 2022, Type Ic supernova event SN 2022jli was observed in NGC 157, reaching a peak magnitude of 14.4.[13]

References

  1. ↑ 1.0 1.1 Skrutskie, Michael F. et al. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal 131 (2): 1163–1183. doi:10.1086/498708. ISSN 0004-6256. Bibcode: 2006AJ....131.1163S. 
  2. ↑ 2.0 2.1 "NGC 157". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+157. 
  3. ↑ 3.0 3.1 3.2 Tully, R. Brent et al. (August 2016). "Cosmicflows-3". The Astronomical Journal 152 (2): 21. doi:10.3847/0004-6256/152/2/50. 50. Bibcode: 2016AJ....152...50T. 
  4. ↑ Moore, T. et al. (October 2023). "SN 2022jli: A Type Ic Supernova with Periodic Modulation of Its Light Curve and an Unusually Long Rise" (in en). The Astrophysical Journal Letters 956 (1): L31. doi:10.3847/2041-8213/acfc25. ISSN 2041-8205. Bibcode: 2023ApJ...956L..31M. 
  5. ↑ 5.0 5.1 5.2 O'Meara, Stephen James (June 14, 2007). Herschel 400 Observing Guide. Cambridge University Press. p. 303. ISBN 9780521858939. https://www.google.com/books/edition/Herschel_400_Observing_Guide/Nyh9fAC_tpIC?gbpv=1&pg=PA303. 
  6. ↑ 6.0 6.1 6.2 Crowther, Paul A. (January 2013). "On the association between core-collapse supernovae and H ii regions". Monthly Notices of the Royal Astronomical Society 428 (3): 1927–1943. doi:10.1093/mnras/sts145. Bibcode: 2013MNRAS.428.1927C. 
  7. ↑ 7.0 7.1 ">New General Catalog Objects: NGC 150 - 199". http://cseligman.com/text/atlas/ngc1a.htm#157. 
  8. ↑ 8.0 8.1 Zobnina, D. I.; Zasov, A. V. (April 2020). "Galaxies with Declining Rotation Curves". Astronomy Reports 64 (4): 295–309. doi:10.1134/S1063772920050054. Bibcode: 2020ARep...64..295Z. 
  9. ↑ Zhu, Ming et al. (December 2009). "Tracing Molecular Gas Mass in Extreme Extragalactic Environments: An Observational Study". The Astrophysical Journal 706 (2): 941–959. doi:10.1088/0004-637X/706/2/941. Bibcode: 2009ApJ...706..941Z. 
  10. ↑ Sempere, M. J.; Rozas, M. (January 1997). "Dynamical model of the grand-design spiral galaxy NGC 157". Astronomy and Astrophysics 317: 405–415. Bibcode: 1997A&A...317..405S. 
  11. ↑ Monard, L. A. G. (May 2009). Green, D. W. E.. ed. "Supernova 2009em in NGC 157". Central Bureau Electronic Telegrams 1798: 1. Bibcode: 2009CBET.1798....1M. 
  12. ↑ Navasardyan, H.; Benetti, S. (May 2009). Green, D. W. E.. ed. "Supernova 2009em in NGC 157". Central Bureau Electronic Telegrams 1806: 1. Bibcode: 2009CBET.1806....1N. 
  13. ↑ "Transient Name Server entry for SN 2022jli". https://www.wis-tns.org/object/2022jli. 

External links



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