Shedding Light on Black Holes
- 18 September 1998
- journal article
- perspective
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 281 (5384) , 1815-1816
- https://doi.org/10.1126/science.281.5384.1815
Abstract
Radio astronomers have long known about extremely strong radiation sources such as Cygnus A and Virgo A, but the origin of the energy has been a mystery. As Reid discusses in his Perspective, astronomers have increasingly come to accept the notion that these bright radio sources are powered by massive black holes. Results reported in the same issue by Hirabayashi et al. add to that understanding. Images taken with the very long baseline interferometry Space Observatory Program (VSOP) show the radio frequency-emitting core of Virgo A in unprecedented detail.This publication has 5 references indexed in Scilit:
- Overview and Initial Results of the Very Long Baseline Interferometry Space Observatory ProgrammeScience, 1998
- Filaments in the radio lobes of M87The Astrophysical Journal, 1989
- The jet and filaments in Cygnus AThe Astrophysical Journal, 1984
- The Brightness Distribution Within the Radio Sources Cygnus A (19N4A) and Cassiopeia A (23N5A)Monthly Notices of the Royal Astronomical Society, 1959
- Fluctuations in Cosmic Radiation at Radio-FrequenciesNature, 1946