Observation of Cosmic Soft X-Rays

Details Observation of Cosmic Soft X-Rays Observation of Cosmic Soft X-Rays

Jul 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972ap%26ss..17...30h&link_type=abstract

Astrophysics and Space Science, Volume 17, Issue 1, pp.30-38

Astronomy and Astrophysics

Astrophysics

19

Scientific paper

Cosmic X-rays in the energy range between 0.2˜10 keV were observed with polypropylene window proportional counters on board a sounding rocket. The field of view crossed the galactic plane in the Sgr region and reached galactic latitudes of 50° and -90°. A new soft X-ray source was found in the Aries-Taurus region. The soft X-ray flux from the direction of NGC 1275 was conspicuous, whereas that of Sgr region source were very weak. The distribution of the intensity of diffuse soft X-rays over the scanned region indicates the galactic emission of soft X-rays.

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