The velocity gradient of B361

Details The velocity gradient of B361 The velocity gradient of B361

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...263..160c&link_type=abstract

Astrophysical Journal, Part 1, vol. 263, Dec. 1, 1982, p. 160-165. Research supported by the Research Corp.

Astronomy and Astrophysics

Astrophysics

8

Gas Dynamics, Interstellar Gas, Nebulae, Velocity Distribution, Angular Momentum, Formaldehyde, Gas Density, Hydroxyl Radicals, Magnetic Effects, Velocity Measurement

Scientific paper

Observations of a well-ordered velocity gradient that decreases with decreasing cloud radius are reported for the galactic dark cloud B361. The source also exhibits systematic changes in spectral line width. Current observations confirm the suggestion of rotation in this source reported earlier and imply the presence of an effective mechanism for redistributing angular momentum. Magnetic braking is invoked to explain the observed effects.

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