Abstract
A new EXOSAT (LE/CMA) observation of the region in Crux (R.A. ∼11h 45m, Dec. ∼-62°) 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 sufficent to distinguish clearly between the assumption of one or two (possibly interacting) SNR's in the region.
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Mereghetti, S., Bignami, G.F., Caraveo, P.A. et al. Some crucial X-ray observations — One or two SNR(s) in Crux?. Space Sci Rev 40, 495–501 (1985). https://doi.org/10.1007/BF00179861
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DOI: https://doi.org/10.1007/BF00179861