A Transient Radio Source near the Center of the Milky Way Galaxy
JUN-HUI ZHAO 1,
D. A. ROBERTS 1,
W. M. GOSS 1,
D. A. FRAIL 1,
K. Y. LO 2,
R. SUBRAHMANYAN 3,
M. J. KESTEVEN 3,
R. D. EKERS 3,
D. A. ALLEN 4,
M. G. BURTON 4, and
J. SPYROMILIO 4
1 National Radio Astronomy Observatory, P.O. Box 0, Socorro, NM 87801
2 Astronomy Department, University of Illinois, 1002 West Green Street, Urbana, Illinois 61801
3 Australia Telescope National Facility, P.O. Box 76, Epping, New South Wales 2121, Australia
4 Anglo Australian Observatory, P.O. Box 296, Epping, New South Wales 2121, Australia
In late December 1990, a new radio source appeared near the center of our galaxy rivaling the intensity of Sgr A* (the compact radio source at the galactic center). Following its first detection, the flux density of the galactic center transient (GCT) increased rapidly to a maximum 1 month later, and then declined gradually with a time scale of about 3 months. Surprisingly, the GCT maintained a steep radio spectrum during both its rising and decay phases. The neutral hydrogen (HI) absorption shows similar absorption to that in front of Sgr A*; this indicates that the GCT lies near the galactic center. Furthermore, both HI and OH observations show an additional deep absorption at +20 kilometers per second with respect to the local standard of rest. Thus, the GCT is either embedded in or located behind a molecular cloud moving with that velocity. The cloud can be seen on infrared images. Its opacity is shown to be inadequate to conceal a supernova near the galactic center. It is argued that the GCT was probably transient radio emission from synchrotron-radiating plasma associated with an x-ray binary system.
Submitted on December 9, 1991
Accepted on February 6, 1992
