Interstellar absorption lines in the galaxy NGC 1705

Details Interstellar absorption lines in the galaxy NGC 1705 Interstellar absorption lines in the galaxy NGC 1705

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...351..412y&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 351, March 10, 1990, p. 412-417.

Astronomy and Astrophysics

Astronomy

30

Dwarf Galaxies, Interstellar Extinction, Ultraviolet Spectra, Absorption Spectra, Interstellar Gas, Local Group (Astronomy)

Scientific paper

The possibility is considered, and shown to be plausible, that the strong C IV and Si IV absorption lines in low-resolution ultraviolet spectra of gas-rich dwarf galaxies are primarily interstellar, not stellar as has been supposed. The argument is based on analogies with H II regions in the Local Group, on low-resolution equivalent width measurements of gas-rich dwarf galaxies from the literature and on high-resolution UV spectra of NGC 1705.

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