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NGC 3175 is a spiral galaxy located in the far eastern part of the southern constellation of Antlia[8] at an approximate distance of 54 million light-years.[5] NGC 3175 was discovered on March 30, 1835 by English astronomer John Herschel,[9] whose notes described it as, "considerably bright, large, much extended NE-SW, very gradually little brighter middle".[10] This galaxy is the namesake of the NGC 3175 group of galaxies,[6] which includes the spiral galaxy NGC 3137.[11]

NGC 3175
NGC 3175 taken by the Hubble Space Telescope[1]
Observation data (J2000[2] epoch)
ConstellationAntlia
Right ascension10h 14m 42.111s[3]
Declination−28° 52′ 19.42″[3]
Redshift0.003613[2]
Helio radial velocity1,081.1 km/s[4]
Distance53.9 Mly (16.52 Mpc)[5]
Group or clusterNGC 3175 group[6]
Apparent magnitude (B)12.08[5]
Characteristics
TypeSAB(s)b[7]
Mass(7.34±0.85)×1010[6] M☉
Mass/Light ratio7.13+1.78
−1.98[6] M☉/L☉
Apparent size (V)5′.0 × 1′.3[8]
Other designations
IRAS 1012-286P13, 2MASX J10144211-2852194, NGC 3175, LEDA 29892, MCG -05-24-028[2]

The morphological classification of this galaxy is SAB(s)b,[7] which indicates a weakly-barred spiral galaxy (SAB) with no inner ring structure (s), and somewhat tightly wound spiral arms (b). It spans an angular size of 5′.0 × 1′.3,[8] with the major axis aligned along a position angle of 56°. The plane of the galaxy is inclined at an angle of 77° to the line of sight from the Earth,[12] and thus is being viewed close to edge on.

A study of the galaxy using the Australia Telescope Compact Array found that the outer disk of this galaxy, beyond a radius of 3.5 kpc from the core, is free of neutral hydrogen emission. This is an indication that no star formation is occurring, which is peculiar for a spiral galaxy. In contrast, the central region is undergoing star formation and contains 5.8×108 M☉ of neutral hydrogen. There are no nearby galaxies that could explain the stripping of hydrogen gas from the outer part of the galaxy.[6]


See also



References


  1. "Galactic Diversity". www.spacetelescope.org. Retrieved 10 December 2019.
  2. "NGC 3175". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-12-10.
  3. Skrutskie, Michael F.; et al. (February 1, 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131: 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256.
  4. Meyer, M. J.; et al. (June 2004). "The HIPASS catalogue - I. Data presentation". Monthly Notices of the Royal Astronomical Society. 350 (4): 1195–1209. arXiv:astro-ph/0406384. Bibcode:2004MNRAS.350.1195M. doi:10.1111/j.1365-2966.2004.07710.x. S2CID 10336076.
  5. Tully, R. Brent; et al. (August 2016). "Cosmicflows-3". The Astronomical Journal. 152 (2): 21. arXiv:1605.01765. Bibcode:2016AJ....152...50T. doi:10.3847/0004-6256/152/2/50. 50.
  6. Dahlem, M.; et al. (May 2001). "The mysterious H I deficiency of NGC 3175". Astronomy and Astrophysics. 371: 45–51. arXiv:astro-ph/0103086. Bibcode:2001A&A...371...45D. doi:10.1051/0004-6361:20010313.
  7. Dahlem, M.; et al. (October 2006). "Dependence of radio halo properties on star formation activity and galaxy mass". Astronomy and Astrophysics. 457 (1): 121–131. arXiv:astro-ph/0607102. Bibcode:2006A&A...457..121D. doi:10.1051/0004-6361:20054787.
  8. Streicher, Magda (June 2010). "Antlia, the Machine Pneumatique". Monthly Notes of the Astronomical Society of South Africa. 69 (5 and 6): 107–112. Bibcode:2010MNSSA..69..107S.
  9. Seligman, C. "NGC 3175 (= PGC 29892 = PGC 736480)". Celestial Atlas. Retrieved 2021-12-18.
  10. Aranda, Ted (November 25, 2011). 3,000 Deep-Sky Objects, An Annotated Catalogue. Springer New York. p. 221. ISBN 9781441994196.
  11. Kondapally, Rohit; Russell, George A.; Conselice, Christopher J.; Penny, Samantha J. (December 2018). "Faint satellite population of the NGC-3175 Group - a Local Group analogue". Monthly Notices of the Royal Astronomical Society. 481 (2): 1759–1773. arXiv:1808.09020. Bibcode:2018MNRAS.481.1759K. doi:10.1093/mnras/sty2333.
  12. Mathewson, D. S.; Ford, V. L. (November 1996). "Parameters of 2447 Southern Spiral Galaxies for Use in the Tully-Fisher Relation". Astrophysical Journal Supplement. 107: 97. Bibcode:1996ApJS..107...97M. doi:10.1086/192356.


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На других языках

[de] NGC 3175

NGC 3175 ist eine Balken-Spiralgalaxie mit ausgedehnten Sternentstehungsgebieten vom Hubble-Typ SBab[2] im Sternbild Antlia am Südsternhimmel. Sie ist rund 40 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 70.000 Lichtjahren. Gemeinsam mit NGC 3113, NGC 3125, NGC 3137 und ESO 499-37 bildet sie die kleine NGC 3175-Gruppe.
- [en] NGC 3175

[ru] NGC 3175

NGC 3175 (другие обозначения — ESO 436-3, IRAS10124-2837, MCG −5-24-28, VV 796, UGCA 207, AM 1012—283, PGC 29892) — спиральная галактика в созвездии Насоса. Открыта Джоном Гершелем в 1835 году[3].


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