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J/A+AS/125/475 DD Mon BV light curves (Qian+ 1997)
Photometric study of the close binary system DD Monocerotis Qian S., Liu Q., Yang Y., Gu S., Huang Z. <Astron. Astrophys. Suppl. Ser. 125, 475 (1997)> =1997A&AS..125..475Q (SIMBAD/NED BibCode)
ADC_Keywords: Binaries, eclipsing ; Photometry Keywords: stars: DD Mon - binaries: eclipsing - stars: fundamental parameters Abstract: New BV light curves of the short-period eclipsing binary system DD Mon have been obtained. Light-curve variability is seen in both B and V bands as compared with the light curves obtained in 1986 by Yamasaki et al. (1990AJ.....99.1218Y). The light curves are analyzed by using Wilson-Devinney's synthetic light-curve program, and the present photometric solution reveals that DD Mon is a near-contact binary with the secondary component filling the Roche lobe. Combined with Yamasaki et al.'s (1990AJ.....99.1218Y) spectroscopic results, absolute quantities of DD Mon are derived: mass of the primary M1=1.05±0.08M☉, mass of the secondary M2=0.47±0.04M☉, radius of the primary R1=1.36±0.04R☉, radius of the secondary R2=1.03±0.03R☉. These results show that the components of DD Mon have evolved away from the ZAMS and through a mass-transfer process to the present semi-detached state. The variation in shape of the light curve may be caused by the evolution of the system and the activity of dark spots. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 06 45 57 -00 16.9 DD Mon = HD 292319 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 18 402 V observations of DD Mon table2 18 358 B observations of DD Mon fig1.ps 82 60024 B and V light curves of DD Mon tables.tex 76 202 LaTeX version of the tables
Byte-by-byte Description of file: table1 table2
Bytes Format Units Label Explanations
1- 11 F11.4 d HJD Heliocentric Julina date 13- 17 F5.3 mag DMag Differential V or B magnitude (1)
Note (1): Differential magnitude between these observations and those obtained in 1986 by Yamasaki et al. (1990AJ.....99.1218Y) V magnitude in table1, B magnitude in table2
Acknowledgements: Yulan Yang
(End) Patricia Bauer [CDS] 11-Apr-1997
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