An optically directed HI search for new dwarf members of the M 81 group

Details An optically directed HI search for new dwarf members of the M 81 group An optically directed HI search for new dwarf members of the M 81 group

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26as..127..269h&link_type=abstract

Astronomy and Astrophysics Supplement, v.127, p.269-276

Astronomy and Astrophysics

Astrophysics

15

Galaxies: Irregular, Radio Lines: Galaxies, Galaxies: M 81, Galaxies Clusters M 81 Group

Scientific paper

We present a search for neutral hydrogen (HI) emission from optically identified dwarf galaxy candidates in the larger M81 group area. Of 136 candidates, 68 galaxies have been detected (this corresponds to a detection rate of ~ 49%). Most of the detected galaxies are background objects and fail to be classified as dwarfs. Many known dwarfs in the M81 group have been detected, but no new members have been discovered.

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