High-resolution observations of the intergalactic H I cloud in the M96 group

Details High-resolution observations of the intergalactic H I cloud in the M96 group High-resolution observations of the intergalactic H I cloud in the M96 group

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986aj.....91...13s&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 91, Jan. 1986, p. 13-22.

Astronomy and Astrophysics

Astronomy

18

Extragalactic Radio Sources, Galactic Clusters, Hydrogen Clouds, Intergalactic Media, Neutral Gases, Astronomical Maps, H Lines, High Resolution, Radial Velocity, Radio Spectra, Very Large Array (Vla), Very Long Base Interferometry

Scientific paper

The large cloud complex of intergalactic H I in the M96 group has been observed with the D array of the Very Large Array. The main cloud has been resolved into a number of clumps which account for most of the H I previously detected at Arecibo. Additionally, high-resolution spectra have been made at Arecibo that show evidence of narrower subcomponents within the ≡30 - 50 km s-1 wide H I profiles previously found at Arecibo. In general, the kinematics of the gas follow the overall pattern found in the original observations, but there are some indications that the clumps may be dynamically independent.

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