The UBV photoelectric lightcurves of the eclipsing binary FS Lupi, observed at ESO, La Silla, during 1982-1984, have been analyzed with a Roche-model-based lightcurve synthesis method. The system, alternatively classified in the past as an EA or EB system, results an A-type contact binary with a relatively large degree of overcontact (33%) and with a large difference in the temperatures of the components (1120 K), which explains the EB-type light curve. The asymmetries and the large scatter of the observed data, when investigated in terms of deviations from the (synthetic) mean light curve, show a systematic trend which has been studied with three different methods, search- ing for periodicity.
FS Lupi: a contact binary in poor thermal contact / Milano, L.; Russo, G.; Terzan, A.. - In: ASTRONOMY & ASTROPHYSICS. - ISSN 0004-6361. - 183:(1987), pp. 265-273.
FS Lupi: a contact binary in poor thermal contact
L. MilanoMembro del Collaboration Group
;G. Russo
Membro del Collaboration Group
;
1987
Abstract
The UBV photoelectric lightcurves of the eclipsing binary FS Lupi, observed at ESO, La Silla, during 1982-1984, have been analyzed with a Roche-model-based lightcurve synthesis method. The system, alternatively classified in the past as an EA or EB system, results an A-type contact binary with a relatively large degree of overcontact (33%) and with a large difference in the temperatures of the components (1120 K), which explains the EB-type light curve. The asymmetries and the large scatter of the observed data, when investigated in terms of deviations from the (synthetic) mean light curve, show a systematic trend which has been studied with three different methods, search- ing for periodicity.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.