Hot interstellar matter in the magellanic clouds

Details Hot interstellar matter in the magellanic clouds Hot interstellar matter in the magellanic clouds

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996uill.rept.....c&link_type=abstract

Technical Report, Illinois Univ. Chicago, IL United States

Physics

Magellanic Clouds, Interstellar Matter, Visual Observation, X Ray Sources, Radio Observation, Ultraviolet Emission, Ionized Gases, Star Clusters, Rosat Mission

Scientific paper

ROSAT PSPC observations of fields in the Large Magellanic Cloud was used
to study the large-scale diffuse x ray emission. The x-ray data was used
in combination with additional information from optical, ultraviolet,
and radio observations to determine the physical nature of observed
diffuse x-ray emmision.

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