An optical counterpart of the giant H I cloud H I 1225 + 0146

Details An optical counterpart of the giant H I cloud H I 1225 + 0146 An optical counterpart of the giant H I cloud H I 1225 + 0146

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...359..302m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 359, Aug. 20, 1990, p. 302-306.

Astronomy and Astrophysics

Astrophysics

20

Dwarf Galaxies, H I Regions, Irregular Galaxies, Molecular Clouds, Brightness Distribution, Emission Spectra, H Ii Regions, Ionized Gases, Schmidt Telescopes

Scientific paper

An investigation based on deep U.K. Schmidt Telescope direct plates has discovered a previously uncataloged dwarf irregular galaxy which, it is proposed, is associated with the 1225 + 0146 extragalactic H I cloud. This new optical feature is characterized by a number of knots embedded in low surface brightness material about 1 arcmin in extent. The object is classified as an M(B) = -15.5 Magellanic type dwarf irregular galaxy about 5 kpc in extent. The brightest knot is considered to be an H II region.

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