Study of the fine structure in a high-positive velocity cloud

Details Study of the fine structure in a high-positive velocity cloud Study of the fine structure in a high-positive velocity cloud

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26as...78..437c&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 78, no. 3, June 1989, p. 437-440.

Astronomy and Astrophysics

Astronomy

3

Fine Structure, Hydrogen Clouds, Sky Surveys (Astronomy), Spectral Resolution, Angular Resolution, Density Distribution, Morphology, Velocity Distribution

Scientific paper

Neutral-hydrogen 21-cm line measurements have been made of the positive-high-velocity cloud HVC 267.5 + 21 + 222 to study its fine structure. Maps of the H I column density distribution, the velocity field, and the distribution of velocity widths are given. The data suggest the presence of two HVCs partially overlapping on the sky. The mass has been estimated as 1475 R squared solar masses, where R is the distance in kpc.

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