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Some crucial X-ray observations — One or two SNR(s) in Crux? (1985)

Mereghetti, S. ; Bignami, G. F. ; Caraveo, P. A. ; [et al.]

Springer

Space science reviews 40 (1985), S. 495-501

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ISSN: 1572-9672

Source: Springer Online Journal Archives 1860-2000

Topics: Physics

Notes: 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.

Type of Medium: Electronic Resource

URL: http://dx.doi.org/10.1007/BF00179861

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