Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...300..675h&link_type=abstract
Astronomy and Astrophysics, v.300, p.675
Astronomy and Astrophysics
Astrophysics
51
Galaxies: Elliptical, Galaxies: Evolution, Galaxies: Interactions, Galaxies: Interstellar Matter, Radio Lines: Atomic
Scientific paper
HI observations are reported for a total of 53 IRAS elliptical galaxies. Nearby confusing sources may be responsible for some of the 33 detections. There are 24 isolated detected galaxies, which can be split into two groups, one having the same M_HI_/L_B_ ratio as the elliptical galaxies from the RSA (M_HI_/L_B_=0.030+/-0.026). A second group is more than six times richer in HI (M_HI_/L_B_=0.206+/-0.105). The "HI-rich" galaxies have blue colors like spiral galaxies and have a tendency towards higher average dust temperatures. The large number of elliptical galaxies in compact groups (in this sample) suggests that gravitational interactions and mergers may be an important source of interstellar matter for elliptical galaxies.
Henkel Carsten
Huchtmeier Walter K.
Sage Leslie J.
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