Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996cuny.rept.....t&link_type=abstract
Technical Report, Columbia Univ. New York, NY United States Columbia Astrophysics Laboratory. Depts. of Asatronomy and Physics.
Astronomy and Astrophysics
Astronomy
X Rays, Gamma Ray Bursts, Gamma Ray Astronomy, Gamma Ray Observatory, Gamma Rays, Radio Stars, Emission Spectra, X Ray Astronomy, Synchrotron Radiation, Light Emission, Massive Stars, Peculiar Stars, Blazars
Scientific paper
The investigation consists of different projects carried out during the Cycle 5 GRO observing phase. EGRET, COMPTEL and BATSE studies of unidentified gamma ray sources resulted in the discovery of a new gamma ray transient near the Galactic plane, GRO J1838-0145. We show that this new transient and the time-variable gamma ray sources GRO J1021-58, GRO J1813-12, and GRO J1828+01, are not associated with radio-loud spectrally flat blazar-like counterparts. A GRO study of the gamma ray source 2CG 135+1 is aimed at studying the time-variable gamma ray emission from the source possible associated with the peculiar radio counterpart/massive star LSI 61 303. A BATSE study of the hard X-ray emission from X-ray bursters aimed at detecting and interpreting this emission. The object Aquila X-1 is of particular importance. We recently discovered a prominent hard X-ray outburst from Aquila X-1 correlated with soft X-ray and optical emission. A study of galactic superluminal X-ray transients discovered several prominent radio flares from GRS 1915+105 that turn out to be strongly correlated with hard X-ray emission. Finally, a new model of gamma-ray burst (GRB) emission is being developed, based on synchrotron emission of impulsively accelerated particles.
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