DETECTION OF AN UNRESOLVED NUCLEAR RADIO-SOURCE IN M31 (VOL 390, PG L9,199 2)

Citation
Pc. Crane et al., DETECTION OF AN UNRESOLVED NUCLEAR RADIO-SOURCE IN M31 (VOL 390, PG L9,199 2), The Astrophysical journal, 411(2), 1993, pp. 120000107-120000107
Citations number
1
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
0004637X
Volume
411
Issue
2
Year of publication
1993
Part
2
Pages
120000107 - 120000107
Database
ISI
SICI code
0004-637X(1993)411:2<120000107:DOAUNR>2.0.ZU;2-U
Abstract
An unresolved radio source with a flux density of 28 +/- 5 muJy has be en detected at the center of the galaxy M31. This source coincides wit h the optical stellar nucleus and with a variable Einstein X-ray sourc e but is only 1/300 as luminous as the Galactic center source Sgr A an d one-fifth as luminous as Sgr A. Consequently, this object is the we akest known nuclear radio source. No evidence is found for radio emiss ion from the remnant of supernova 1885A in M31. An upper limit of 15 m uJy (3 sigma) has been determined for the flux density of this source, which is 1/15 the value for Tycho's SNR if it were at the same distan ce.