On the Observation of Double Stars for the Determination of Their Proper Motions

Details On the Observation of Double Stars for the Determination of Their Proper Motions On the Observation of Double Stars for the Determination of Their Proper Motions

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.110..117z&link_type=abstract

Astrophysics and Space Science, Volume 110, Issue 1, pp.117-118

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The state of meridian observations of the DS (double stars) program is reported. The program contains close double stars whose precise positions can be determined by the visual method only. In some declination zones these stars have been observed at a few observatories of the USSR and in Strasbourg, Santiago de Chile and Beograd. The importance of further DS observations, particularly in the southern sky, is stressed.

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