Relative radial velocities of stars determined from GPO spectrograms.

Details Relative radial velocities of stars determined from GPO spectrograms. Relative radial velocities of stars determined from GPO spectrograms.

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979msngr..17...29g&link_type=abstract

The Messenger, vol. 17, p. 29-32

Astronomy and Astrophysics

Astronomy

1

Radial Velocities:Stars

Scientific paper

One of the first telescopes to be installed on La Silla was the GPO 40 cm astrograph. Although it is one of the "smallest" instruments at the ESO observatory, it is by no means less productive than the larger ones! On the contrary, the impressive results that have recently been obtained by Dr. Frank Gieseking of the Hoher List Observatory, near Bonn, proves the tremendous potential of this instrument. Thanks to the good accuracy of the measured radial velocities, large-scale investigations of stellar motions can now be carried out.

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