Search for duplicity in periodic variable Be stars

Details Search for duplicity in periodic variable Be stars Search for duplicity in periodic variable Be stars

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...385..488c&link_type=abstract

Astronomy and Astrophysics, v.385, p.488-502 (2002)

Astronomy and Astrophysics

Astrophysics

4

Stars: Emission-Line, Be, Stars: Binaries: Spectroscopic, Stars: Individual: Hr 1960, Hr 2968, Hr 3237, Hr 3642

Scientific paper

Four Be stars, HR 1960, HR 2968, HR 3237 and HR 3642, selected according to their periodic variations in HIPPARCOS and GENEVA photometries, were monitored from 1998 until 2001 with the CORALIE spectrograph. Among these stars, two are new spectroscopic binaries and one is a new lambda Eri short period variable. HR 1960 is a low amplitude (K = 3.4 km s-1) SB1 with a period of 395.48 d in agreement with the photometric prediction. HR 3237 is a short period SB1 (P = 5.1526 d). HR 3642 presents some interesting variations in photometry and spectroscopy: indeed, a mid- and a short-term variation is present with periods of 137.99 d (Hp magnitude) and 1.13028 d (radial velocity) respectively. The short-term variation, characteristic of the lambda Eri stars, probably implies non-radial pulsations or inhomogeneities in the corotating disc. The last star, HR 2968, is an excellent photometric binary candidate, but no spectroscopic obviousness of a companion has been found. Based on observations collected at the Swiss 40 cm, 70 cm and 120 cm telescopes at the European Southern Observatory (La Silla, Chile) and on data from the ESA HIPPARCOS satellite. The photometric and radial velocity data are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/385/488 Table 3 is only available in electronic form at http://www.edpsciences.org

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