Bibcode
Desmet, M.; Frémat, Y.; Baudin, F.; Harmanec, P.; Lampens, P.; Pacheco, E. Janot; Briquet, M.; Degroote, P.; Neiner, C.; Mathias, P.; Poretti, E.; Rainer, M.; Uytterhoeven, K.; Amado, P. J.; Valtier, J.-C.; Prša, A.; Maceroni, C.; Aerts, C.
Bibliographical reference
Monthly Notices of the Royal Astronomical Society, Volume 401, Issue 1, pp. 418-432.
Advertised on:
1
2010
Citations
35
Refereed citations
28
Description
Analyses of very accurate CoRoT space photometry, past Johnson V
photoelectric photometry and high-resolution echelle spectra led to the
determination of improved and consistent fundamental stellar properties
of both components of AU Monocerotis. We derived new, accurate
ephemerides for both the orbital motion (with a period of ) and the
long-term, overall brightness variation (with a period of ) of this
strongly interacting Be + G semi-detached binary. It is shown that this
long-term variation must be due to attenuation of the total light by
some variable circumbinary material. We derived the binary mass ratio
MG/MB = 0.17 +/- 0.03 based on the assumption that
the G-type secondary fills its Roche lobe and rotates synchronously.
Using this value of the mass ratio as well as the radial velocities of
the G-star, we obtained a consistent light curve model and improved
estimates of the stellar masses, radii, luminosities and effective
temperatures. We demonstrate that the observed lines of the B-type
primary may not be of photospheric origin. We also discover rapid and
periodic light changes visible in the high-quality residual CoRoT light
curves. AU Mon is put into perspective by a comparison with known
binaries exhibiting long-term cyclic light changes.
Based on photometry collected by the CoRoT space mission as well as
spectroscopy obtained with the FEROS spectrograph attached to the 2.2-m
telescope at European Southern Observatory (ESO), La Silla, Chile, under
the ESO Large Programme LP178.D-0361, and with the SOPHIE spectrograph
of the Observatoire de Haute-Provence (France). The CoRoT space mission
was developed and is operated by the French space agency CNES, with the
participation of ESA's RSSD and Science Programmes, Austria, Belgium,
Brazil, Germany and Spain. Based on observations collected at the Centro
Astronómico Hispano Alemán (CAHA) at Calar Alto, operated
jointly by the Max-Planck-Institut für Astronomie and the Instituto
de Astrofísica de Andalucía (CSIC).
E-mail: maarten.desmet [at] ster.kuleuven.be (maarten[dot]desmet[at]ster[dot]kuleuven[dot]be)