Some crucial X-ray observations - One or two SNR(s) in crux?

Details Some crucial X-ray observations - One or two SNR(s) in crux? Some crucial X-ray observations - One or two SNR(s) in crux?

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ssrv...40..495m&link_type=abstract

(ESA, ESLAB Symposium on X-Ray Astronomy in the EXOSAT Era, 18th, The Hague, Netherlands, Nov. 5-9, 1984) Space Science Reviews

Astronomy and Astrophysics

Astronomy

1

Supernova Remnants, X Ray Astronomy, Astronomical Maps, Diffuse Radiation, Exosat Satellite, Radio Astronomy

Scientific paper

A new Exosat (LE/CMA) observation of the region in Crux (R.A. of approximately 11 h 45 m, Dec. of approximately -62 deg) where Markert et al. (1981) reported the existence of two X-ray SNR's is presented. After 'cleaning' the CMA field from the point source component due to the UV emission of the numerous stars in the field, the smoothed X-ray contours are compared to the 408 MHz radio map of Caswell et al. (1983). The existence of two well-separate X-ray emission regions is confirmed by Exosat, and the current X-ray/radio picture is not sufficient to distinguish clearly between the assumption of one or two (possibly interacting) SNR's in the region.

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