H I in early-type galaxies. III - Observations of S0 galaxies

Details H I in early-type galaxies. III - Observations of S0 galaxies H I in early-type galaxies. III - Observations of S0 galaxies

Nov 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...209..710b&link_type=abstract

Astrophysical Journal, vol. 209, Nov. 1, 1976, pt. 1, p. 710-715. Research supported by the National Radio Astronomy Observator

Astronomy and Astrophysics

Astronomy

47

Galactic Evolution, Galactic Structure, Hydrogen, Radio Sources (Astronomy), Spiral Galaxies, Astronomical Catalogs, Color, Stellar Magnitude, Ubv Spectra

Scientific paper

Observations of H I in 17 selected early-type galaxies (predominantly S0) are reported. The H I mass-to-light ratio is roughly correlated with galaxy color (based on B-V photometry) but not with other characteristics of these galaxies. Morphologically normal S0 galaxies display the same general trend between H I mass-to-light ratio and color as that followed by normal galaxies along the Hubble sequence and by peculiar and Irr II galaxies as well.

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