Evidence for a Black Hole in a Radio-Quiet Quasar Nucleus
Author(s) -
Katherine M. Blundell,
A. J. Beasley,
Mark Lacy,
S. T. Garrington
Publication year - 1996
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/310242
Subject(s) - quasar , merlin (protein) , quiet , physics , astrophysics , brightness , astronomy , jet (fluid) , active galactic nucleus , brightness temperature , core (optical fiber) , black hole (networking) , radio galaxy , galaxy , optics , computer science , routing protocol , link state routing protocol , medicine , computer network , routing (electronic design automation) , cancer , suppressor , thermodynamics
We present the first milli-arcsecond resolution radio images of a radio-quietquasar, detecting a high brightness temperature core with data from the VLBA.On maps made with lower-frequency data from MERLIN and the VLA jets appear toemanate from the core in opposite directions, which correspond toradio-emission on arcsecond scales seen with the VLA at higher frequencies.These provide strong evidence for a black-hole--based jet-producing centralengine, rather than a starburst, being responsible for the compact radioemission in this radio-quiet quasar.
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom