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NGC 7331, also known as Caldwell 30, is an unbarred spiral galaxy about 40 million light-years (12 Mpc) away in the constellation Pegasus. It was discovered by William Herschel in 1784.[3] NGC 7331 is the brightest galaxy in the field of a visual grouping known as the NGC 7331 Group of galaxies. In fact, the other members of the group, NGC 7335, 7336, 7337 and 7340, lie far in the background at distances of approximately 300-350 million light years.[4]

NGC 7331
Observation data (J2000 epoch)
ConstellationPegasus
Right ascension22h 37m 04.1s[1]
Declination+34° 24′ 56″[1]
Redshift816 ± 1 km/s[1]
Distance39.8 ± 3.3 Mly (12.2 ± 1.0 Mpc) [2]
Apparent magnitude (V)10.4[1]
Characteristics
TypeSA(s)b[1]
Size120,000 ly (diameter)
Apparent size (V)10′.5 × 3′.7[1]
Other designations
UGC 12113, PGC 69327,[1] Caldwell 30
Image of a supernova that appeared in the galaxy in 2014 (called 2014C). The inset images are from NASA's Chandra X-ray Observatory, showing a small region of the galaxy before the supernova explosion (left) and after it (right). Red, green and blue colors are used for low, medium and high-energy X-rays, respectively.
Image of a supernova that appeared in the galaxy in 2014 (called 2014C). The inset images are from NASA's Chandra X-ray Observatory, showing a small region of the galaxy before the supernova explosion (left) and after it (right). Red, green and blue colors are used for low, medium and high-energy X-rays, respectively.

The galaxy appears similar in size and structure to the Milky Way, and is sometimes referred to as "the Milky Way's twin".[5] However, discoveries in the 2000s regarding the structure of the Milky Way may call this similarity into doubt, particularly because the latter is now believed to be a barred spiral, compared to the unbarred status of NGC 7331.[6] In spiral galaxies the central bulge typically co-rotates with the disk but the bulge in the galaxy NGC 7331 is rotating in the opposite direction to the rest of the disk.[7] In both visible light and infrared photos of the NGC 7331, the core of the galaxy appears to be slightly off-center, with one side of the disk appearing to extend further away from the core than the opposite side.

Multiple supernova events have been observed in this galaxy. SN 1959D, a Type IIL supernova,[8] was the first supernova identified within NGC 7331.[1] The supernova was discovered by Milton Humason and H. S. Gates in a survey at Palomar Observatory.[9] More recent supernovae are SN 2013bu and SN 2014C, the latter of which underwent an unusual "metamorphosis" from a hydrogen-poor Type Ib to a hydrogen-rich Type IIn over the course of a year . [10] A 1903 photographic plate from Yerkes Observatory shows a magnitude 16.6 candidate transient that may have also been a supernova.[11]


See also



References


  1. "NASA/IPAC Extragalactic Database". Results for NGC 7331. Retrieved 2006-11-10.
  2. Jensen, Joseph B.; Tonry, John L.; Barris, Brian J.; Thompson, Rodger I.; et al. (February 2003). "Measuring Distances and Probing the Unresolved Stellar Populations of Galaxies Using Infrared Surface Brightness Fluctuations". Astrophysical Journal. 583 (2): 712–726. arXiv:astro-ph/0210129. Bibcode:2003ApJ...583..712J. doi:10.1086/345430. S2CID 551714.
  3. The NGC/IC Project Archived 2011-02-28 at the Wayback Machine : NGC Discoverers List by Bob Erdmann.
  4. "Spiral Galaxy NGC 7331, Galaxy Group (NGC 7335, 7336, 7337)".
  5. "Seeing Double: Spitzer Captures Our Galaxy's Twin". Spitzer Space Telescope Newsroom. Spitzer Science Center. 2004-06-28. Archived from the original on May 17, 2007. Retrieved 2008-04-24.
  6. "The Milky Way Has Only Two Spiral Arms". 2008-06-03. Retrieved 2008-06-04.
  7. A Counter-rotating Bulge in the Sb Galaxy NGC 7331 , F. Prada, C. Gutierrez, R.F. Peletier, C.D. McKeith, the Astrophysical Journal, 463 :L9–L12, 20/5/1996
  8. "NASA/IPAC Extragalactic Database". Results for SN 1959D. Retrieved 2006-11-10.
  9. M. L. Humason; H. S. Gates (1960). "The 1959 Palomar Supernova Search". Publications of the Astronomical Society of the Pacific. 72 (426): 208–209. Bibcode:1960PASP...72..208H. doi:10.1086/127513.
  10. D. Milisavljevic; et al. (2015). "Metamorphosis of SN 2014C: Delayed Interaction Between a Hydrogen Poor Core-collapse Supernova and a Nearby Circumstellar Shell". The Astrophysical Journal. 815 (2): 120. arXiv:1511.01907. Bibcode:2015ApJ...815..120M. doi:10.1088/0004-637X/815/2/120. S2CID 31773513.
  11. Cerny; Chapman; Glusman; Kron; Liang; et al. (2021). "Precise Photometric Measurements from a 1903 Photographic Plate Using a Commercial Scanner". Publications of the Astronomical Society of the Pacific. arXiv:2101.03699.



На других языках

[de] NGC 7331

NGC 7331 ist eine Spiralgalaxie vom Hubble-Typ Sbc im Sternbild Pegasus am Nordsternhimmel. Sie ist schätzungsweise 46 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Scheibendurchmesser von etwa 140.000 Lj. Im selben Himmelsareal befindet sich u. a. die Zwerggalaxie NGC 7337.
- [en] NGC 7331

[es] NGC 7331

NGC 7331 es una galaxia espiral en la constelación de Pegaso, localizada 9° al noroeste de Scheat (β Pegasi). De magnitud aparente 10,4 puede ser observada con pequeños telescopios. Descubierta por William Herschel en 1784, es una de las galaxias más brillantes que no están incluidas en el catálogo Messier.

[ru] NGC 7331

NGC 7331 (другие обозначения — PGC 69327, UGC 12113, MCG 6-49-45, ZWG 514.68) — спиральная галактика в созвездии Пегаса. Находится на расстоянии около 43 миллионов световых лет от Солнца. Была открыта Уильямом Гершелем в 1784 году.


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