Optical observations of the radio star Beta Persei with the Paris Observatory astrolabe from 1980 to 1983

Details Optical observations of the radio star Beta Persei with the Paris Observatory astrolabe from 1980 to 1983 Optical observations of the radio star Beta Persei with the Paris Observatory astrolabe from 1980 to 1983

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26as...63..305d&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 63, no. 2, Feb. 1986, p. 305, 306. In French.

Astronomy and Astrophysics

Astrophysics

2

Astrolabes, Radio Stars, Stellar Spectrophotometry, Visible Spectrum, Error Analysis, Mean Square Values, Position (Location), Reference Stars, Tables (Data), Transit Time

Scientific paper

The first five systematic campaigns of optical positions for the radio star β Persei began, at the astrolabe of the Paris Observatory, in 1975 (Debarbat et al., 1981). Three more campaigns have been performed; the limits of the observations, their number at both (east and west) transits are given in table I. Table II gives the Δα and Δδ(with the meaning "Astrolabe-FK4") together with the mean square error for each campaign. The more or less abnormal value in declination for the 1982/1983 campaign could be the result of the limited number of observations at both transits. β Persei is one of the radiostars to be used for linking of "radio" and "optical" reference system.

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