X-ray emission from supergiant shell in the LMC.

Details X-ray emission from supergiant shell in the LMC. X-ray emission from supergiant shell in the LMC.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..237b&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 237 - 238

Astronomy and Astrophysics

Astrophysics

1

Magellanic Clouds: X Rays, Magellanic Clouds: Shells

Scientific paper

The authors have used the Snowden & Petre (1995) mosaics of pointed ROSAT PSPC observations of the Large Magellanic Cloud to study the X-ray characteristics of supergiant shells. Diffuse soft X-ray emission above the background is detected in all of the well-defined supergiant shells. The observed large range of X-ray properties can be explained by differential obscuration, temperature and density differences, and localized heating by supernova remnants.

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