The optical counterpart to the large H I cloud in Virgo

Details The optical counterpart to the large H I cloud in Virgo The optical counterpart to the large H I cloud in Virgo

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aj....101.1258s&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 101, April 1991, p. 1258-1274.

Other

75

Dwarf Galaxies, Galactic Evolution, H I Regions, Irregular Galaxies, Virgo Galactic Cluster, Abundance, Astronomical Spectroscopy, Brightness Distribution, Emission Spectra, Star Formation, Ubv Spectra

Scientific paper

Detailed imaging and spectroscopic observations of the optical counterpart to H I 1225 + 01 are reported, as are the results of 2.6-mm CO observations. Nebular abundances are derived, and a number of models are presented in an attempt to account for both the chemical and photometric color evolution of this galaxy. The physical properties of the galaxy are then discussed, and various scenarios for its evolutionary status are considered by comparing the observed parameters with model predictions and similar quantities for other galaxies.

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