J/other/NewA/34.253      Light curves of 8 Algol-type systems     (Zasche, 2015)

First analysis of eight Algol-type systems: V537 And, GS Boo, AM CrB, V1298 Her, EL Lyn, FW Per, RU Tri, and WW Tri. Zasche P. <New Astron., 34, 253 (2015)> =2015NewA...34..253Z 2015NewA...34..253Z
ADC_Keywords: Binaries, eclipsing Keywords: stars: binaries: eclipsing -- stars: fundamental parameters Abstract: Analyzing available photometry from the Super WASP and other databases, we performed the very first light curve analysis of eight eclipsing binary systems V537 And, GS Boo, AM CrB, V1298 Her, EL Lyn, FW Per, RU Tri, and WW Tri. All of these systems were found to be detached ones of Algol-type, having the orbital periods of the order of days. 722 new times of minima for these binaries were derived and presented, trying to identify the period variations caused by the third bodies in these systems. Description: The target selection for this paper was rather straightforward. We have chosen only these systems, which are known to be eclipsing variables, their orbital period is known, has never been analysed before and have enough photometric data points for an analysis. Thanks to the good time coverage provided by the Super WASP survey we used this database for the whole analysis. All of the analysed systems are the northern-hemisphere stars (DE>20°) of moderate brightness (9.5mag<V<13mag) and with the orbital periods ranging from 0.6 to 3.3 days. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file stars.dat 59 8 List of studied stars minima.dat 41 722 List of the minima timings used for the analysis -------------------------------------------------------------------------------- Byte-by-byte Description of file: stars.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Star Name of the star 11- 12 I2 h RAh Simbad Hour of Right Ascension (J2000.0) 14- 15 I2 min RAm Simbad Minute of Right Ascension (J2000.0) 17- 21 F5.2 s RAs Simbad Second of Right Ascension (J2000.0) 23 A1 --- DE- Simbad Sign of the Declination (J2000.0) 24- 25 I2 deg DEd Simbad Degree of Declination (J2000.0) 27- 28 I2 arcmin DEm Simbad Arcminute of Declination (J2000.0) 30- 33 F4.1 arcsec DEs Simbad Arcsecond of Declination (J2000.0) 35- 39 F5.2 mag Bmag Simbad B band magnitude 41- 45 F5.2 mag Vmag ? Simbad V band magnitude 47- 55 F9.7 d Per [0.6/3.3] Period 57- 59 I3 --- Nmin [36/135] Number of minima, in minima.dat file -------------------------------------------------------------------------------- Byte-by-byte Description of file: minima.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Star Name of the star 11- 21 F11.5 d HJD [51200/55002] Heliocentric Julian Date of minimum (HJD-2400000) 23- 29 F7.5 d e_HJD [0/0.07] Error of HJD 31- 34 A4 --- Type [Prim Sec] Type of minimum (primary/secondary) 36 A1 --- Filter [CVW] Filter used (C fir NSVSn W for WASP) 38- 41 A4 --- Ref Source (1) -------------------------------------------------------------------------------- Note (1): Sources as follows: WASP = WASP, Pollacco et al., 2006PASP..118.1407P 2006PASP..118.1407P NSVS = NSVS, Wozniak et al., 2004AJ....127.2436W 2004AJ....127.2436W ASAS = ASAS, Pojmanski, 2002AcA....52..397P 2002AcA....52..397P, Cat. II/264 -------------------------------------------------------------------------------- Acknowledgements: Petr Zasche, petr.zasche(at)email.cz References: WASP, Pollacco et al., 2006PASP..118.1407P 2006PASP..118.1407P NSVS, Wozniak et al., 2004AJ....127.2436W 2004AJ....127.2436W ASAS, Pojmanski, 2002AcA....52..397P 2002AcA....52..397P
(End) Patricia Vannier [CDS] 13-Jan-2015
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