A very high velocity H I cloud in the direction of M31

Details A very high velocity H I cloud in the direction of M31 A very high velocity H I cloud in the direction of M31

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975mnras.170p..45d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 170, Mar. 1975, p. 45P-49P.

Astronomy and Astrophysics

Astronomy

25

Andromeda Galaxy, Hydrogen Clouds, Radio Astronomy, Velocity Distribution, Astronomical Maps, Galactic Evolution, Galactic Structure, Magellanic Clouds, Nebulae, Radio Telescopes

Scientific paper

A neutral hydrogen cloud with a velocity of -447 km per sec relative to the local standard of rest has been discovered near the direction of the Andromeda nebula (M31). Observations with the Mark IA radio telescope show that its half-power dimensions are 0.40 deg x 0.36 deg; it is situated approximately 1.5 deg NW of the center of M31. Two alternative theories of the origin of this cloud are discussed.

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