Astronomy:NGC 5735

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NGC 5735
NGC 5735 imaged by SDSS
Observation data (J2000 epoch)
ConstellationBoötes
Right ascension 14h 42m 33.2479s[1]
Declination+28° 43′ 35.420″[1]
Redshift0.012408±0.00000700[1]
Helio radial velocity3,720±2 km/s[1]
Distance190.48 ± 2.45 Mly (58.400 ± 0.751 Mpc)[2]
Group or clusterNGC 5653 Group (LGG 383)
Apparent magnitude (V)13.10[1]
Characteristics
TypeSB(rs)bc[1]
Size~155,200 ly (47.57 kpc) (estimated)[1]
Apparent size (V)2.4′ × 1.9′[1]
Other designations
IRAS 14403+2856, UGC 9481, MCG+05-35-007, PGC 52535[1]

NGC 5735 is a barred spiral galaxy in the constellation of Boötes. Its velocity with respect to the cosmic microwave background is 3,894±12 km/s, which corresponds to a Hubble distance of 187.3 ± 13.1 Mly (57.44 ± 4.02 Mpc).[1] Additionally, three non-redshift measurements give a similar mean distance of 190.48 ± 2.45 Mly (58.400 ± 0.751 Mpc).[2] It was discovered by German-British astronomer William Herschel on 17 May 1784.[3][4]

NGC 5735 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.[5][6]

NGC 5653 group

NGC 5735 is a member of the NGC 5653 group (also known as LGG 383). This group contains 15 galaxies, including NGC 5629, NGC 5635 (fr), NGC 5639 (fr), NGC 5641, NGC 5642, NGC 5653, NGC 5659 (fr), NGC 5657 (fr), NGC 5672 (fr), NGC 5703 (fr), IC 4397, UGC 9253 (d), UGC 9268 (d), and UGC 9302 (d).[7][8]

Supernova

One supernova has been observed in NGC 5735:

See also

References

  1. ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 "Results for object NGC 5735". NASA and Caltech. https://ned.ipac.caltech.edu/byname?objname=NGC+5735. 
  2. ↑ 2.0 2.1 "Distance Results for NGC 5735". NASA. https://ned.ipac.caltech.edu/cgi-bin/nDistance?name=NGC+5735. 
  3. ↑ Herschel, William (1786). "Catalogue of One Thousand New Nebulae and Clusters of Stars". Philosophical Transactions of the Royal Society of London 76: 457–499. doi:10.1098/rstl.1786.0027. Bibcode: 1786RSPT...76..457H. https://zenodo.org/record/1432282/files/article.pdf. 
  4. ↑ Seligman, Courtney. "New General Catalogue Objects: NGC 5735". https://cseligman.com/text/atlas/ngc57.htm#5735. 
  5. ↑ Toba, Y.; Oyabu, S.; Matsuhara, H.; Malkan, M. A.; Gandhi, P.; Nakagawa, T.; Isobe, N.; Shirahata, M. et al. (2014). "Luminosity and Redshift Dependence of the Covering Factor of Active Galactic Nuclei viewed with WISE and Sloan Digital Sky Survey". The Astrophysical Journal 788 (1): 45. doi:10.1088/0004-637X/788/1/45. Bibcode: 2014ApJ...788...45T. 
  6. ↑ "NGC 5735". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+5735. 
  7. ↑ Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series 100: 47. Bibcode: 1993A&AS..100...47G. 
  8. ↑ "LGG 383". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=LGG+383. 
  9. ↑ Nakano, S.; Naito, H.; Shimada, M.; Takaki, T.; Yamaoka, H. (2006). "Supernova 2006qp in NGC 5735". Central Bureau Electronic Telegrams (764): 1. Bibcode: 2006CBET..764....1N. http://www.cbat.eps.harvard.edu/iau/cbet/000700/CBET000764.txt. 
  10. ↑ "SN 2006qp". IAU. https://www.wis-tns.org/object/2006qp. 

Coordinates: Sky map 14h 42m 33.2479s, +28° 43′ 35.420″



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