H I observations of Shostak's high-velocity cloud

Details H I observations of Shostak's high-velocity cloud H I observations of Shostak's high-velocity cloud

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.182..395c&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 182, Feb. 1978, p. 395-399.

Astronomy and Astrophysics

Astronomy

14

Galactic Structure, Hydrogen Clouds, Intergalactic Media, Interstellar Gas, Angular Resolution, Cosmic Dust, Dwarf Stars, Magellanic Clouds, Size Determination

Scientific paper

The high-velocity cloud at 39.4 deg galactic longitude, +4.7 deg galactic latitude reported by Shostak (1977) has been surveyed in the 21-cm hydrogen line at high sensitivity with an angular resolution of 12 arcmin and a velocity resolution of 1.8 km/s. The cloud consists of a small core with a tail elongated perpendicular to the galactic plane. Possible interpretations of the object are discussed, and it is suggested that the object may be an intergalactic gas cloud associated with the Local Group of galaxies.

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