X-ray emission from superbubbles.

Details X-ray emission from superbubbles. X-ray emission from superbubbles.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..241c&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 241 - 242

Astronomy and Astrophysics

Astrophysics

1

Magellanic Clouds: Interstellar Bubbles, Interstellar Bubbles: Supernova Remnants, Interstellar Bubbles: X Rays

Scientific paper

X-ray emission from superbubbles can be used to determine the physical condition of the superbubble interior, place constraints on the ambient interstellar medium, and diagnose the existence of supernova remnant shocks. ROSAT observations of superbubbles in the Large Magellanic Cloud have provided the first useful X-ray spectra for the bright objects and useful upper limits on the faint objects.

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