The tail of M33 and the adjacent hydrogen cloud

Details The tail of M33 and the adjacent hydrogen cloud The tail of M33 and the adjacent hydrogen cloud

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...233...35w&link_type=abstract

Astrophysical Journal, Part 1, vol. 233, Oct. 1, 1979, p. 35-38.

Astronomy and Astrophysics

Astronomy

22

Galactic Structure, Hydrogen Clouds, Radio Sources (Astronomy), Spiral Galaxies, Astronomical Maps, Centimeter Waves, Emission Spectra, Galactic Radiation

Scientific paper

New observations are presented of the outskirts of M33 and of the adjacent high-velocity hydrogen cloud. M33 has an H I tail which is probably a part of the warped hydrogen disk of that galaxy. The adjacent H I cloud has a southern extension but no material connection with M33. Various extragalactic hypotheses for the cloud are discussed in relation to the tail and warp of M33, but the cloud is probably associated with other high-velocity hydrogen clouds in this general direction.

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