astro.wikisort.org - Galaxy

Search / Calendar

IC 167 is a barred spiral galaxy in the constellation of Aries. It was first reported by Bigourdan in 1891[1] and included in Dreyer's first Index Catalogue.[2]

IC 167
NGC 691 (upper left) and IC 167 (lower right)
Observation data (J2000 epoch)
ConstellationAries
Right ascension01h 51m 08.65s
Declination+21° 54 44.8
Redshift0.00982 ± 0.00017
Apparent magnitude (V)14.0
Characteristics
TypeSBc
Apparent size (V)3.09 × 1.862
Other designations
Arp 31, LEDA 6833, MCG+04-05-021, Z 0148.3+2140, APG 31, 2MASX1 J0151084+215447, UGC 1313, Z 482-25, LCSB L76, 2MASX J01510855+2154461, UZC J015108.6+215445

Galaxy group information


IC 167 is a member of the NGC 697 group.[3] There is some evidence that IC 167 is interacting with nearby NGC 694 as they seem to share HI regions.[3] The tidal warping of IC 167 also is indicative of an interaction with another galaxy.[3] How long the interaction between these two galaxies has been occurring is the subject of current research.[4]


References


  1. Bigourdan, Guillaume (1891). "Nebuleuses nouvelles, decouvertes a l'Obseratoire de Paris" (PDF). Comptes rendus hebdomadaires des séances de l'Académie des Sciences. 112: 647–650. Archived from the original (PDF) on 26 July 2011. Retrieved 29 December 2010.
  2. Dreyer, J.L.E. (1895). "Index Catalogue of Nebulae found in the years 1888 to 1894, with Notes and Corrections to the New General Catalogue". Mem. R. Astron. Soc. 51: 185–228. Bibcode:1895MmRAS..51..185D. Archived from the original on 2010-02-20. Retrieved 29 December 2010.
  3. van Moorsel, G.A. (1988). "A neutral hydrogen study of interacting galaxies in the NGC 697 group". Astronomy & Astrophysics. 202: 59–69. Bibcode:1988A&A...202...59V.
  4. Iyer, Mansie G.; Simpson, Caroline E.; Gottesman, Stephen T.; Malphrus, Benjamin K. (September 2004). "Neutral hydrogen in ARP 158". Astronomical Journal. 128 (3): 985–996. arXiv:astro-ph/0405405. Bibcode:2004AJ....128..985I. doi:10.1086/422731. S2CID 17323672.



На других языках


[de] IC 167

IC 167 = Arp 31 ist eine Balken-Spiralgalaxie vom Hubble-Typ SBc im Sternbild Widder auf der Ekliptik. Sie ist schätzungsweise 136 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 105.000 Lichtjahren.
- [en] IC 167



Текст в блоке "Читать" взят с сайта "Википедия" и доступен по лицензии Creative Commons Attribution-ShareAlike; в отдельных случаях могут действовать дополнительные условия.

Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.

2019-2025
WikiSort.org - проект по пересортировке и дополнению контента Википедии