On the rotation of star clusters and nebulae as determined from radial velocities

Details On the rotation of star clusters and nebulae as determined from radial velocities On the rotation of star clusters and nebulae as determined from radial velocities

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...240..803n&link_type=abstract

Astrophysical Journal, Part 1, vol. 240, Sept. 15, 1980, p. 803.

Astronomy and Astrophysics

Astrophysics

2

Nebulae, Radial Velocity, Rotation, Star Clusters, Angular Velocity, Galactic Rotation, Globular Clusters, Milky Way Galaxy, Stellar Rotation

Scientific paper

The fictitious apparent rotation due to a body's tangential velocity is
unimportant for Galactic nebulae, but it may be important for globular
clusters and the high-velocity clouds.

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