From Wikipedia, the free encyclopedia
3C 371
Hubble Legacy Archive Near- UV image of the jet coming out of 3C 371
Observation data ( Epoch J2000)
Constellation Draco
Right ascension18h 06m 50.681s [1]
Declination+69° 49′ 28.11″ [1]
Redshift0.051 [1] [2]
Distance730 million light-years
224 M pc [3]
Type BL Lac [1] [2] [3]
FRI RG [4]
Apparent magnitude (V)14.4 [2] ±1.5 [5]
Other designations
UGC 11130, PGC 61417, 2E 4023, 7C 180717.90+694858.00, QSO B1807+698 [1]
See also: Quasar, List of quasars

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

  1. ^ a b c d e f "3C 371". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2010-04-11.
  2. ^ a b c d e "NASA/IPAC Extragalactic Database". Results for 3C 371. Retrieved 2010-04-11.
  3. ^ a b c "3C 371". XJET: X-Ray Emission from Extragalactic Radio Jets. 2008-01-11. Retrieved 2010-04-11.
  4. ^ 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.
  5. ^ 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.


From Wikipedia, the free encyclopedia
3C 371
Hubble Legacy Archive Near- UV image of the jet coming out of 3C 371
Observation data ( Epoch J2000)
Constellation Draco
Right ascension18h 06m 50.681s [1]
Declination+69° 49′ 28.11″ [1]
Redshift0.051 [1] [2]
Distance730 million light-years
224 M pc [3]
Type BL Lac [1] [2] [3]
FRI RG [4]
Apparent magnitude (V)14.4 [2] ±1.5 [5]
Other designations
UGC 11130, PGC 61417, 2E 4023, 7C 180717.90+694858.00, QSO B1807+698 [1]
See also: Quasar, List of quasars

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

  1. ^ a b c d e f "3C 371". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2010-04-11.
  2. ^ a b c d e "NASA/IPAC Extragalactic Database". Results for 3C 371. Retrieved 2010-04-11.
  3. ^ a b c "3C 371". XJET: X-Ray Emission from Extragalactic Radio Jets. 2008-01-11. Retrieved 2010-04-11.
  4. ^ 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.
  5. ^ 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.



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