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NGC 2775

From Wikipedia, the free encyclopedia
Galaxy in the constellation Cancer
NGC 2775
NGC 2775 imaged by theHubble Space Telescope
Observation data (J2000epoch)
ConstellationCancer
Right ascension09h 10m 20.112s[1]
Declination+07° 02′ 16.53″[1]
Redshift1,316.4±13.4 km/s[2]
Distance67 Mly (20.5 Mpc)[3]
Apparent magnitude (V)10.4[4]
Characteristics
TypeSAa[5] or SA(r)ab[6]
Apparent size (V)4.3 × 3.3[6]
Other designations
UGC 4820,[7]PGC 25861,[8]Caldwell 48

NGC 2775, also known asCaldwell 48, is aspiral galaxy in theconstellationCancer. It is 67 millionlight-years (20.5megaparsecs)[3] away from theMilky Way. It was discovered byWilliam Herschel in 1783. NGC 2775 belongs to theAntlia-Hydra Cluster[9] of galaxies and is the most prominent member of the NGC 2775 Group, a smallgalaxy group in theVirgo Super-cluster, along with theLocal Group. Other members of the NGC 2775 Group includeNGC 2777 andUGC 4781.[10]

This object has amorphological classification of SA(r)ab,[6] which indicates anunbarred spiral galaxy (SA) with a prominent ring structure (r) andflocculent,[11] tightly woundspiral arms (ab).[12] The galaxy is inclined by an angle of 44° to theline of sight from theEarth.[6] The galactic nucleus is notactive[2] and the largenuclear bulge, which extends out to an angular radius of0.4′,[12] is relatively gas free.[11] An explanation for the latter could be a highsupernova rate.[6] Althoughstar formation is taking place in the dusty outer ring,[12] NGC 2775 does not display any currentstarburst activity,[13] and the galactic nucleus is virtually free of any star formation whatsoever.[11]

The galaxy's hydrogen tail feature indicates a past interaction with a faint companion.[6] Asatellite galaxy appears to have orbited NGC 2775 multiple times, losing mass as it does so and creating faint, shell-like structures.[12] Nearby irregular galaxy NGC 2777 displays a tidal tail of hydrogen gas that points back to NGC 2775, suggesting the two may be linked.[14]

One supernova has been observed in NGC 2775. SN 1993Z (type Ia, mag. 13.9) was discovered by theLeuschner Observatory Supernova Search (LOSS) on 23 September 1993.[15][16] By September 25, spectral analysis showed that it had peaked about four weeks earlier.[15]

Gallery

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  • NGC 2775 imaged with a 32-inch telescope.
    NGC 2775 imaged with a 32-inch telescope.
  • Map showing the location of NGC 2775.
    Map showing the location of NGC 2775.
  • NGC 2775 (SDSS DR14)
    NGC 2775 (SDSS DR14)
  • NGC 2775 from the Hubble Space Telescope
    NGC 2775 from theHubble Space Telescope

References

[edit]
  1. ^abSkrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 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.
  2. ^abvan den Bosch, Remco C. E.; et al. (May 2015). "Hunting for Supermassive Black Holes in Nearby Galaxies With the Hobby-Eberly Telescope".The Astrophysical Journal Supplement Series.218 (1): 13.arXiv:1502.00632.Bibcode:2015ApJS..218...10V.doi:10.1088/0067-0049/218/1/10.S2CID 117876537. 10.
  3. ^abCappellari, Michele; et al. (May 2011)."The ATLAS3D project - I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria".Monthly Notices of the Royal Astronomical Society.413 (2):813–836.arXiv:1012.1551.Bibcode:2011MNRAS.413..813C.doi:10.1111/j.1365-2966.2010.18174.x.S2CID 15391206.
  4. ^Finlay, Warren H. (2014).Concise Catalog of Deep-sky Objects. The Patrick Moore Practical Astronomy Series (2nd ed.). Springer Science & Business Media. p. 227.ISBN 978-3-319-03169-9.
  5. ^Ann, H. B.; et al. (2015). "A Catalog of Visually Classified Galaxies in the Local (z ~ 0.01) Universe".The Astrophysical Journal Supplement Series.217 (2):27–49.arXiv:1502.03545.Bibcode:2015ApJS..217...27A.doi:10.1088/0067-0049/217/2/27.S2CID 119253507.
  6. ^abcdefHogg, David E.; et al. (March 2001)."Hot and Cold Gas in Early-Type Spirals: NGC 3623, NGC 2775, and NGC 1291".The Astronomical Journal.121 (3):1336–1357.Bibcode:2001AJ....121.1336H.doi:10.1086/319400.
  7. ^"NGC 2775".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2020-04-19.
  8. ^"NASA/IPAC Extragalactic Database".Results for NGC 2775. Retrieved2010-03-24.
  9. ^O'Meara, Stephen James; Moore, Patrick (2002).The Caldwell objects (2nd ed.). Sky Publishing Corporation. p. 192.ISBN 0521827965.
  10. ^"A List of Nearby Galaxy Groups".Atlas of the Universe. Retrieved2010-11-28.
  11. ^abc"Hubble Spots Feathered Spiral".NASA. 2020-07-02. Retrieved2020-07-03.
  12. ^abcdKönig, Michael; Binnewies, Stefan (2017).The Cambridge Photographic Atlas of Galaxies. Cambridge University Press. p. 35.ISBN 978-1107189485.
  13. ^Shapiro, Kristen L.; et al. (December 2003). "Observational Constraints on Disk Heating as a Function of Hubble Type".The Astronomical Journal.126 (6):2707–2716.arXiv:astro-ph/0308489.Bibcode:2003AJ....126.2707S.doi:10.1086/379306.S2CID 15388910.
  14. ^Arp, Halton; Sulentic, Jack W. (July 1991). "The Properties of NGC 2777: Are Companion Galaxies Young?".Astrophysical Journal.375: 569.Bibcode:1991ApJ...375..569A.doi:10.1086/170218.
  15. ^abTreffers, R. R.; Filippenko, A. V.; Leibundgut, B.; Paik, Y.; Lee, L. F. M.; Richmond, M. W. (1993). "Supernova 1993Z in NGC 2775".International Astronomical Union Circular (5870): 3.Bibcode:1993IAUC.5870....3T.
  16. ^"SN 1993Z".Transient Name Server.IAU. Retrieved7 December 2024.

External links

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