VLA/GBI observations of the new high mass X-ray binary LS 5039

Details VLA/GBI observations of the new high mass X-ray binary LS 5039 VLA/GBI observations of the new high mass X-ray binary LS 5039

Nov 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999newar..43..545r&link_type=abstract

New Astronomy Reviews, Volume 43, Issue 8-10, p. 545-547.

Astronomy and Astrophysics

Astronomy

4

Scientific paper

We comment on the main radio emitting properties of the proposed high mass X-ray binary LS 5039. Our study is based on multi-epoch observations with the VLA radio interferometer, at 2.0, 3.6, 6.0 and 20 cm wavelengths, as well as on the first data obtained by the GBI-NASA Monitoring Program at 3.6 and 13.3 cm wavelengths. The source appears to be compact (θ<=0''.1) and moderately variable, with a non-thermal radio spectrum suggestive of synchrotron radiation.

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