J/AJ/146/35               BVR light curves of DZ Psc               (Yang+, 2013)

Deep, low mass ratio overcontact binary systems. XIII. DZ Piscium with intrinsic light variability. Yang Y.-G., Qian S.-B., Zhang L.-Y., Dai H.-F., Soonthornthum B. <Astron. J., 146, 35 (2013)> =2013AJ....146...35Y 2013AJ....146...35Y
ADC_Keywords: Binaries, eclipsing ; Photometry, UBVRI Keywords: binaries: eclipsing - stars: activity - stars: individual: DZ Psc Abstract: New multi-color photometry for the eclipsing binary DZ Psc was performed in 2011 and 2012 using the 85cm telescope at the Xinglong Station of the National Astronomical Observatories of China. Using the updated Wilson-Devinney (W-D) code, we deduced two sets of photometric solutions. The overcontact degree is f=89.7(±1.0)%, identifying DZ Psc as a deep, low mass ratio overcontact binary. The asymmetric light curves (i.e., LC2 in 2012) were modeled by a hot spot on the primary star. Based on all of the available light minimum times, we discovered that the orbital period of DZ Psc may be undergoing a secular period increase with a cyclic variation. The modulated period and semi-amplitude of this oscillation are Pmod=11.89(±0.19)yr and A=0.0064(±0.0006)days, which may be possibly attributed to either cyclic magnetic activity or light-time effect due to the third body. The long-term period increases at a rate of dP/dt=+7.13(±0.17)*10-7days/yr, which may be interpreted as conserved mass transfer from the less massive component to the more massive one. With mass transferring, DZ Psc will finally merge into a rapid-rotation single star when Jspin/Jorb>1/3. Description: New multi-color photometry of DZ Psc was performed on several nights during two observing seasons from 2011 December 22 to 2012 December 31, using the 85cm telescope at the Xinglong Station (XLs) of the National Astronomical Observatories of China (NAOC). The standard Johnson/Cousins set of BVIR filters was mounted. Three primary eclipses of DZ Psc were monitored on 2009 December 6 and 2011 November 19 using the 1.0m telescope and on 2011 December 30 using the 60cm telescope at Yunnan Astronomical Observatory (YNAO) in China. Objects: ------------------------------------------------------------------ RA (ICRS) DE Designation(s) (Period) ------------------------------------------------------------------ 00 36 27.94 +21 32 14.4 DZ Piscium = V* DZ Psc (P=0.3661278) ------------------------------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1a.dat 59 347 BVR observations of the contact binary DZ Psc in 2011 table1b.dat 59 554 BVR observations of the contact binary DZ Psc in 2012 table3.dat 29 40 Newly obtained eclipsing times for DZ Psc table4.dat 55 53 All available light minimum times of DZ Psc refs.dat 70 13 References -------------------------------------------------------------------------------- See also: B/gcvs : General Catalogue of Variable Stars (Samus+ 2007-2013) B/vsx : AAVSO International Variable Star Index VSX (Watson+, 2006-2013) V/119 : Catalogue of field contact binary stars (Pribulla+, 2003) J/AJ/143/122 : VR light curves of CK Boo (Yang+, 2012; Paper XII) J/AJ/141/44 : V396 Mon BVRI light curves (Liu+, 2011) J/MNRAS/412/1787 : Physical parameters of 62 eclipsing binaries (Deb+, 2011) J/AJ/131/621 : A catalog of 1022 bright contact binary stars (Gettel+, 2006) J/AJ/130/2252 : VRI photometry of V410 Aur (Yang+, 2005; Paper IV) J/AJ/143/122 : VR light curves of CK Boo (Yang+, 2012) Byte-by-byte Description of file: table1[ab].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 F12.4 d HJD-B ? Heliocentric Julian Date of B band observation 14- 19 F6.3 mag DBmag ? Differential B band magnitude 21- 32 F12.4 d HJD-V Heliocentric Julian Date of V band observation 34- 39 F6.3 mag DVmag Differential V band magnitude 41- 52 F12.4 d HJD-R ? Heliocentric Julian Date of R band observation 54- 59 F6.3 mag DRmag ? Differential R band magnitude -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Ne [1/19] Eclipse number 4- 16 F13.5 d HJD Heliocentric Julian Date (1) 18- 19 A2 --- Min [I /II] Type of minimum (I=primary, II=secondary) 21- 27 F7.5 d e_HJD Uncertainty on HJD 29 A1 --- Flt [BVRI] Filter (B, V, R or I) -------------------------------------------------------------------------------- Note (1): Calculated from new observations and those from Gazeas et al. (2005AcA....55..123G 2005AcA....55..123G) using the method of Kwee & van Woerden (1956BAN....12..327K 1956BAN....12..327K). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 F12.4 d HJD Heliocentric Julian Date 14- 21 F8.1 --- E Eclipse number (.5 for secondary minimum) 23- 25 A3 --- Meth Detection method (vi=visual, pe=photoelectric, CCD) 27- 28 A2 --- Min [I /II] Type of minimum (I=primary, II=secondary) 30- 36 F7.4 d O-C1 The (O-C)1 residual (1) 38- 44 F7.4 d O-C2 The (O-C)2 residual (2) 46- 52 F7.4 d O-C ? Final residual 54- 55 I2 --- Ref [1/13] Reference; in refs.dat file -------------------------------------------------------------------------------- Note (1): Computed using the Kreiner's (2004, cat. J/AcA/54/207) linear ephemeris: MinI=HJD2452500.0842+0.3661278*E. Note (2): From the ephemeris: MinI=HJD2452500.0905(19)+0.36613159(31)*E. -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Ref [1/13] Reference number 4- 22 A19 --- BibCode Bibliographic code 24- 44 A21 --- Aut Author's name 46- 70 A25 --- Com Comments -------------------------------------------------------------------------------- History: From electronic version of the journal References: Qian & Yang, Paper I., 2004AJ....128.2430Q 2004AJ....128.2430Q Zhu et al., Paper II., 2005AJ....129.2806Z 2005AJ....129.2806Z Qian et al., Paper III., 2005AJ....130..224Q 2005AJ....130..224Q Yang et al., Paper IV., 2005AJ....130.2252Y 2005AJ....130.2252Y, Cat. J/AJ/130/2252 Qian et al., Paper V., 2005AJ....130.1206Q 2005AJ....130.1206Q Qian et al., Paper VI., 2006AJ....131.3028Q 2006AJ....131.3028Q Qian et al., Paper VII., 2007AJ....134.1475Q 2007AJ....134.1475Q Qian et al., Paper VIII., 2008AJ....136.1940Q 2008AJ....136.1940Q Yang et al., Paper IX., 2009AJ....138..540Y 2009AJ....138..540Y Qian et al., Paper X., 2011AJ....141..151Q 2011AJ....141..151Q Zhu et al., Paper XI., 2011AJ....142..124Z 2011AJ....142..124Z Yang et al., Paper XII., 2012AJ....143..122Y 2012AJ....143..122Y, Cat. J/AJ/143/122
(End) Greg Schwarz [AAS], Sylvain Guehenneux [CDS] 24-Jun-2014
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line