Access to Astronomical Catalogues

← Click to display the menu
J/AJ/136/594        BS Cas BVR light curves                  (Yang+, 2008)

A photometric study of the neglected eclipsing binary BS Cassiopeiae. Yang Y.-G., Wei J.-Y., He J.-J. <Astron. J., 136, 594-601 (2008)> =2008AJ....136..594Y
ADC_Keywords: Binaries, eclipsing ; Photometry, CCD ; Photometry, UBVRI Keywords: binaries: close - binaries: eclipsing - stars: individual (BS Cassiopeiae) Abstract: We present multicolor charge-coupled device (CCD) photometry for the eclipsing binary BS Cassiopeiae, observed on four nights between 2007 December and 2008 January. Using the Wilson-Devinney program, the photometric solution was derived from our BVR observations. Photometric results indicated that BS Cas is a W-subtype binary, whose mass ratio and overcontact degree are q=0.2834(±0.0010) and f=31.6%(±1.1%), respectively. Light curves of BS Cas present a typical O'Connell effect, which may be attributed to dark spot activity of the primary component. Description: Photoelectric observations of BS Cas were made with the 85cm telescope at Xinglong Station of the National Astronomical Observatories of the Chinese Academy of Sciences (NAOC), equipped with a primary-focus multicolor CCD photometer. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 01 21 38.6 +59 10 27 BS Cas = 2MASS J01213857+5910268 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 56 455 CCD photometric observations in BVR-bands for the eclipsing binary BS Cas table4.dat 64 70 Available light minimum times
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 12 F12.4 d HJD-B ? Heliocentric Julian Date of B band observation 14- 18 F5.3 mag DBmag ? Differential B band magnitude 20- 31 F12.4 d HJD-V ? Heliocentric Julian Date of V band observation 33- 37 F5.3 mag DVmag ? Differential V band magnitude 39- 50 F12.4 d HJD-R Heliocentric Julian Date of R band observation 52- 56 F5.3 mag DRmag Differential R band magnitude
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 Cycle number 23- 25 A3 --- Met Method used: ccd, pg (photographic) or vi (visual) 27- 28 A2 --- Min [I II] Minimum (I or II) 31- 37 F7.4 d (O-C)1 (O-C) from Eq. (2) (1) 39- 45 F7.4 d (O-C)2 (O-C) from Eq. (3) (1) 47- 53 F7.4 d (O-C)3 ? (O-C) from Eq. (5) (1) 55- 61 F7.4 d (O-C)4 ? (O-C) from Eq. (6) (1) 63- 64 I2 -- Ref Reference (2)
Note (1): * For O-C1 and O-C2: Min.I=HJD2427984.7395+0.44047629*E (O-C)1=-0.0270(±0.0007)+7.81(±0.01)x10-6E-1.48(±0.01)x10-10E2 (O-C)2=-0.0005(±0.0002) +0.0023(±0.0014)*sin[5.72(±0.24)E+4.4736(±1.3565)] * For (O-C)3 and (O-C)4: Min.I=HJD2454489.3850(±0.0042)+0.44046828(±0.00000008)*E. (O-C)3=60.2617(±0.0002)+9.81(±0.01)*10-6E-0.91(±0.01)*10-10E2 (O-C)4=-0.0000(±0.0002) +0.0018(±0.0010)*sin[5.79(±0.26)E+3.7177(±1.4380)] Note (2): References as follows: 1 = Ahnert et al. (1947VeSon...1...43A) 2 = Huebscher et al. (1992, BAV Mitt., 60) 3 = Huebscher (2005IBVS.5643....1H) 4 = Blaettler (1997, BBSAG Bull., 114, 5) 5 = Diethelm (1998, BBSAG Bull., 117, 4) 6 = Blaettler (2001, BBSAG Bull., 125, 3) 7 = Dvorak (2003IBVS.5378....1D) 8 = Krajci (2005IBVS.5592....1K) 9 = Pribulla et al. (2005IBVS.5668....1P) 10 = Huebscher et al. (2005IBVS.5657....1H) 11 = Sobotka (2007IBVS.5809....1S) 12 = Dvorak (2006IBVS.5677....1D) 13 = Kim et al. (2006IBVS.5694....1K) 14 = Huebscher & Walter (2007IBVS.5761....1H) 15 = Huebscher et al. (2006IBVS.5731....1H) 16 = Parimucha et al. (2007IBVS.5777....1P) 17 = Dogru et al. (2007IBVS.5795....1D) 18 = Brat et al. (2007, Open Eur. J. Variable Stars, 74, 1) 19 = Present work
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 12-Feb-2011
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

catalogue service

© UDS/CNRS

Contact