Properties of interstellar gas along the line of sight toward SN1987A

Details Properties of interstellar gas along the line of sight toward SN1987A Properties of interstellar gas along the line of sight toward SN1987A

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281b.203w&link_type=abstract

In ESA, Proceedings of the Celebratory Symposium on a Decade of UV Astronomy with the IUE Satellite, Volume 2 p 203-206 (SEE N89

Astronomy and Astrophysics

Astronomy

1

Interstellar Gas, Iue, Magellanic Clouds, Spaceborne Astronomy, Supernova 1987A, Ultraviolet Astronomy, Ultraviolet Spectra, Gas Temperature, Interstellar Extinction

Scientific paper

Results from a coordinated study of optical and UV absorption-line
profiles seen toward SN1987a in the Large Magellanic Cloud (LMC) are
presented. The gas at velocities intermediate between that associated
with either our own Galaxy or the LMC appears to be warm (10,000 K) and
only slightly depleted.

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