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A&A 448, 283-292 (2006)
DOI: 10.1051/0004-6361:20053177
Separation of composite spectra: the spectroscopic detection of an eclipsing binary star
J. F. González and H. LevatoComplejo Astronómico El Leoncito (CASLEO), San Juan, Argentina
e-mail: fgonzalez@casleo.gov.ar
(Received 1 April 2005 / Accepted 5 October 2005)
Abstract
We present an iterative method that allows us to compute the individual
spectra and radial velocities of the two stellar components of spectroscopic binaries.
We applied this method to
HD 143511
and detected the occurrence
of eclipses at the conjunction phases.
The orbital analysis provides minimum masses
with errors of 1%. Absolute masses and radii were derived in two different ways: a) by combining information provided by radial velocities, rotational velocities,
and spectral line intensities; and b) using light curves from the ASAS-3 database.
Key words: techniques: radial velocities -- stars: binaries: spectroscopic -- stars: fundamental parameters -- stars: individual: HD 143511 -- Galaxy: open clusters and associations: individual: NGC 6025
SIMBAD Objects
© ESO 2006
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