3C 371 is a BL Lac object[1][2] located in the constellation Draco. With a redshift of 0.051,[2] this active galaxy is about 730 million light-years away.[3]
3C 371 is a well known object, first associated with the BL Lac class by Miller in 1975,[4] and is among the nearest and brightest BL Lacs.[4] Optical jet emission from 3C 371 was first detected in ground-based images by Nilsson et al. in 1997, and confirmed with HST (Scarpa et al.) in 1999.[4] The implied viewing angle may be less than 18 degrees.[4] But no superluminal motion has been detected, despite frequent monitoring by the Very Long Baseline Array (VLBA).[4]
There are photos of this object dating back to 1895, and they suggest that this objects magnitude can vary by ±1.5.[5]
References
- ^ a b c d e f "3C 371". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2010-04-11.
- ^ a b c d e "NASA/IPAC Extragalactic Database". Results for 3C 371. Retrieved 2010-04-11.
- ^ a b c "3C 371". XJET: X-Ray Emission from Extragalactic Radio Jets. 2008-01-11. Retrieved 2010-04-11.
- ^ a b c d e f Perlin, Eric S.; Padgett; Georganopoulos; Sparks; Biretta; et al. (2006). "Optical Polarimetry of the Jets of Nearby Radio Galaxies. I. The Data". The Astrophysical Journal. 651 (2): 735–748. arXiv:astro-ph/0606119. Bibcode:2006ApJ...651..735P. doi:10.1086/506587. S2CID 53073859.
- ^ a b Usher, Peter D.; Manley, Oscar P. (1968). "The Unusual Long-Term Behavior of 3c 371". Astrophysical Journal. 151: L79 – L82. Bibcode:1968ApJ...151L..79U. doi:10.1086/180147.
External links
- Wikisky image of 3C 371
- New X-ray Jet in Nearby BL Lacertae Object 3C371 (Brandeis University Radio Astronomy)
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