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3C 249.1

Topic: Astronomy

 From HandWiki - Reading time: 5 min

Short description: Galaxy in the constellation Draco
3C 249.1
SDSS image of 3C 249.1
Observation data (Epoch J2000)
ConstellationDraco
Right ascension 11h 04m 13.8777s[1]
Declination+76° 58′ 58.170″[1]
Redshift0.311500[2]
Distance1,194 megaparsecs (3.89×109 ly) h−10.73[2]
TypeSy1, Rad, QSO, X, IR, G, BH?, AG?, UV, gam[1]
QSO[2]
Apparent magnitude (V)15.72[1]
Other designations
LEDA 2821945, 4C 77.09, QSO B1100+773, PG 1100+772
See also: Quasar,List of quasars]]

3C 249.1 is a Seyfert galaxy located in the constellation Draco. It hosts a powerful radio source[3] and is located at redshift 0.3115, with a peculiar radio structure. One of its radio lobes is classified as having a Fanaroff-Riley classification Type II, while the other lobe has no features nor containing hotspots.[4]

3C 249.1 contains emission lines[5] with an extended emission-line region.[6] Its black hole is known to have a high accretion rate.[7]

The star formation rate in 3C 249.1 is estimated to be between ranges of ~1–250 M⊙ yr−1, according to researchers using spectral energy distributions, as well as high resolution mid-infrared spectra of quasars from the Palomar–Green sample.[8]

  • 3C 249.1 observed in radiowaves
    3C 249.1 observed in radiowaves

References

  1. ↑ 1.0 1.1 1.2 1.3 "Query : 3C 249.1". Centre de Données astronomiques de Strasbourg. https://simbad.u-strasbg.fr/simbad/sim-id?Ident=3C+249.1. 
  2. ↑ 2.0 2.1 2.2 "NED results for object 3C 249.1". http://nedwww.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=3C+249.1&extend=no. 
  3. ↑ Lonsdale, C. J.; Morison, I. (1983-05-01). "Asymmetries in four powerful radio sources.". Monthly Notices of the Royal Astronomical Society 203 (3): 833–851. doi:10.1093/mnras/203.3.833. ISSN 0035-8711. Bibcode: 1983MNRAS.203..833L. 
  4. ↑ Marecki, A. (2012-09-01). "Are 3C 249.1 and 3C 334 restarted quasars?" (in en). Astronomy & Astrophysics 545: A132. doi:10.1051/0004-6361/201220010. ISSN 0004-6361. Bibcode: 2012A&A...545A.132M. https://www.aanda.org/articles/aa/abs/2012/09/aa20010-12/aa20010-12.html. 
  5. ↑ Richstone, D. O.; Oke, J. B. (1977-04-01). "The nebulosity near the quasar 3C 249.1.". The Astrophysical Journal 213: 8–14. doi:10.1086/155121. ISSN 0004-637X. Bibcode: 1977ApJ...213....8R. https://ui.adsabs.harvard.edu/abs/1977ApJ...213....8R. 
  6. ↑ Fu, Hai; Stockton, Alan (2006-10-10). "Integral Field Spectroscopy of the Extended Emission-Line Region of 3C 249.1*" (in en). The Astrophysical Journal 650 (1): 80. doi:10.1086/507418. ISSN 0004-637X. Bibcode: 2006ApJ...650...80F. https://iopscience.iop.org/article/10.1086/507418/meta. 
  7. ↑ Yang, Xiaolong; Yao, Su; Yang, Jun; Ho, Luis C.; An, Tao; Wang, Ran; Baan, Willem A.; Gu, Minfeng et al. (2020-12-01). "Radio Activity of Supermassive Black Holes with Extremely High Accretion Rates". The Astrophysical Journal 904 (2): 200. doi:10.3847/1538-4357/abb775. ISSN 0004-637X. Bibcode: 2020ApJ...904..200Y. 
  8. ↑ Xie, Yanxia; Ho, Luis C.; Zhuang, Ming-Yang; Shangguan, Jinyi (2021-04-01). "The Infrared Emission and Vigorous Star Formation of Low-redshift Quasars". The Astrophysical Journal 910 (2): 124. doi:10.3847/1538-4357/abe404. ISSN 0004-637X. Bibcode: 2021ApJ...910..124X. 

Coordinates: Sky map 11h 04m 13.687s, +76° 58′ 58.02″



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