X-ray sources in the Aquila-Serpens-Scutum region

Details X-ray sources in the Aquila-Serpens-Scutum region X-ray sources in the Aquila-Serpens-Scutum region

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.175p..39s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 175, May 1976, p. 39P-46P. Research supported by the Science Research C

Astronomy and Astrophysics

Astronomy

52

Galactic Radiation, Satellite Observation, X Ray Sources, Ariel Satellites, Data Reduction, Graphs (Charts), Sky Surveys (Astronomy), Supernova Remnants, Uhuru Satellite

Scientific paper

The Ariel-5 sky survey detectors have been used to study X-ray sources within 10 deg of the galactic plane between longitudes 20 deg and 55 deg. Seventeen sources have been found and locations and strengths derived. These are compared with results of previous surveys. Seven of these sources were already known and this observation yields an improved position for four of them. Ten of the sources are new. One is possibly associated with the globular cluster NGC 6712, and one with the supernova remnant, W50.

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