Ultraviolet interstellar absorption lines from low-z galaxies

Details Ultraviolet interstellar absorption lines from low-z galaxies Ultraviolet interstellar absorption lines from low-z galaxies

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..408..129s&link_type=abstract

The ultraviolet universe at low and high redshift. AIP Conference Proceedings, Volume 408, pp. 129-133 (1997).

Other

Dwarf Galaxies, Magellanic Clouds And Other Irregular Galaxies, Physical Properties, Ultraviolet

Scientific paper

The importance of studying absorption lines from z<<0.1 galaxies are discussed. The Mg II λλ2796 and 2803 Å doublet absorption is sensitive to low column density gas and has been used to search for absorption lines from low-z galaxies. Recent studies of abundances and depletion patterns toward the Small Magellanic Cloud (Welty et al. 1997) and the NGC 1705 sightline (Sahu & Blades, 1997) are reviewed.

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