Volume 422, Number 3, August II 2004
|Page(s)||1023 - 1029|
|Section||Stellar structure and evolution|
|Published online||16 July 2004|
Institute of Astronomy, Bulgarian Academy of Sciences, 72 Tsarigradsko Shosse Blvd., 1784 Sofia, Bulgaria e-mail: firstname.lastname@example.org
2 Royal Observatory of Belgium, Av. Circulaire 3, 1180 Brussels, Belgium e-mail: Anton.Strigachev@oma.be;Patricia.Lampens@oma.be
Accepted: 13 April 2004
We present accurate CCD astrometric and photometric data for 31 nearby visual double stars in the standard filters BVRI. The observations were collected with a 1.3-m telescope in 2001–2002. The results consist of relative astrometric positions (epoch, angular separation and position angle) and differential BVRI photometry of the components. Mean errors are: 0.01´´ for the separation; 0.06° for the position angle; and 0015 for the photometric data. Comparing the relative positions at different epochs, we evaluate the physical association of the systems. We additionally derive fractional masses and true separations for the most probable binary systems and, whenever orbits are available, also total and component masses.
Key words: stars: binaries: visual / techniques: photometric / stars: fundamental parameters
Table [see full textsee full text] is only available in the electronic form at http:www.edpsciences.org. Tables [see full textsee full text] and [see full textsee full text] are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (18.104.22.168) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/422/1023
© ESO, 2004
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.