Proper motions of galaxies - the reference frame.

Details Proper motions of galaxies - the reference frame. Proper motions of galaxies - the reference frame.

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996msngr..83...29t&link_type=abstract

The Messenger, vol. 83, p. 29-31

Astronomy and Astrophysics

Astronomy

1

Galaxies: Reference Systems, Galaxies: Proper Motions

Scientific paper

CCD astrometry offers the possibility of measuring proper motions for the nearest galaxies, either from the ground or using HST, in only 5 - 10 years. An inertial reference frame, however, is needed against which to measure these motions. The authors have therefore been using the La Silla telescopes to seek QSOs behind several of the nearest satellite galaxies of the Milky Way, using a variety of techniques.

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