IUE observations of N V, a diagnostic of hot interstellar gas

Details IUE observations of N V, a diagnostic of hot interstellar gas IUE observations of N V, a diagnostic of hot interstellar gas

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.192p..73s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 192, Sept. 1980, p. 73P-77P.

Astronomy and Astrophysics

Astronomy

3

Gas Density, High Temperature Gases, Hot Stars, Interstellar Gas, Iue, Nitrogen Ions, Absorption Spectra, Abundance, Emission Spectra, Evaporation, Gas Ionization, Line Spectra, Wolf-Rayet Stars

Scientific paper

The paper reports IUE observations of interstellar N V toward a number
of Wolf-Rayet stars and compares the derived number density with that
predicted by one theory of the interstellar medium. The observed N V/O
VI ratio implies that most of the hot gas in the interstellar medium is
at T about 2.3 x 10 to the 5th K.

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