DOI QR코드

DOI QR Code

The BINSYN Program Package

  • Linnell, Albert P. (Department of Astronomy, University of Washington)
  • Received : 2012.03.02
  • Accepted : 2012.05.01
  • Published : 2012.06.15

Abstract

The BINSYN program package, recently expanded to calculate synthetic spectra of cataclysmic variables, is being further extended to include synthetic photometry of ordinary binary stars in addition to binary stars with optically thick accretion disks. The package includes a capability for differentials correction optimization of eclipsing binary systems using synthetic photometry.

Keywords

References

  1. Bessell MS, UBVRI passbands, PASP, 102, 1181-1199 (1990). http://dx.doi.org/10.1086/132749
  2. Bessell MS, Castelli F, Plez B, Model atmospheres broad-band colors, bolometric corrections and temperature calibrations for O-M stars, A&A, 333, 231-250 (1998). Erratum in A&A, 337, 321 (1998).
  3. Linnell AP, A light synthesis program for binary stars. I, ApJS, 54, 17-31 (1984). http://dx.doi.org/10.1086/190917
  4. Linnell AP, A light synthesis program for binary stars. III - Differential corrections, ApJ, 342, 449-462 (1989). http://dx.doi.org/10.1086/167604
  5. Linnell AP, Harmanec P, Koubsky P, Bozic H, Yang S, et al., Properties and nature of Be stars. 24. Better data and model for the Be+F binary V360 Lacertae, A&A, 455, 1037-1052 (2006). http://dx.doi.org/10.1051/0004-6361:20053792
  6. Linnell AP, Hubeny I, A spectrum synthesis program for binary stars, ApJ, 434, 738-746 (1994). http://dx.doi.org/10.1086/174776
  7. Linnell AP, Hubeny I, A spectrum synthesis and light synthesis program for binary stars with optically thick accretion disks, ApJ, 471, 958-966 (1996). http://dx.doi.org/10.1086/178022
  8. Linnell AP, Godon P, Hubeny I, Sion EM, Szkody P, et al., Synthetic spectrum constraints on a model of the cataclysmic variable QU Carinae, ApJ, 676, 1226-1239 (2008a). http://dx.doi.org/10.1086/529118
  9. Linnell AP, Godon P, Hubeny I, Sion EM, Szkody P, Modeling UX ursae majoris: an abundance of challenges, ApJ, 688, 568-582 (2008b). http://dx.doi.org/10.1086/592104
  10. Linnell AP, Godon P, Hubeny I, Sion EM, Szkody P, The anomalous accretion disk of the cataclysmic variable RW Sextantis, ApJ, 719, 271-286 (2010a). http://dx.doi.org/10.1088/0004-637X/719/1/271
  11. Linnell AP, Szkody P, Plotkin RM, Holtzman J, Seibert M, et al., GALEX and optical light curves of WX LMi, SDSSJ103100.5+202832.2, and SDSSJ121209.31+013627.7, ApJ, 713,1183-1191 (2010b). http://dx.doi.org/10.1088/0004-637X/713/2/1183
  12. Szkody P, Linnell AP, Campbell RK, Plotkin RM, Harrison TE, et al., GALEX, optical, and infrared light curves of MQ Dra: UV excesses at low accretion rates, ApJ, 683, 967-977 (2008). http://dx.doi.org/10.1086/589138

Cited by

  1. Phenomenological Modeling of Newly Discovered Eclipsing Binary 2MASS J18024395 + 4003309 = VSX J180243.9+400331 vol.32, pp.2, 2015, https://doi.org/10.5140/JASS.2015.32.2.127