Hostname: page-component-7dd5485656-frp75 Total loading time: 0 Render date: 2025-10-31T07:59:51.086Z Has data issue: false hasContentIssue false
  • English
  • Français

Be stars in the X-ray binary context

Published online by Cambridge University Press:  30 December 2019

Thomas Rivinius
Thomas Rivinius*
Affiliation:
ESO — European Organisation for Astronomical Research in the Southern Hemisphere, Casilla 19001, Santiago 19, Chile email: triviniu@eso.org
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Rapidly rotating B-type stars with gaseous mass-loss disks in Keplerian rotation are common central objects in X-Ray binaries. These disks are physically well understood in the framework of the viscous decretion disk, and their typical parameters have been established for a large number of single Be stars in the recent years. According to the current observational evidence, the Be stars and disks found in BeXRBs are well within the boundaries known from single Be stars, i.e., they are normal Be stars. New results have also been obtained on the orbital disk truncation and other tidal effects of the companion objects on the disk.

Keywords

circumstellar matterstars: emission-lineBe

References

Bjorkman, K. S., Miroshnichenko, A. S., McDavid, D., & Pogrosheva, T. M. 2002, ApJ, 573, 812 CrossRefGoogle Scholar
Carciofi, A. C., Okazaki, A. T., Le Bouquin, J.-B., et al. 2009, A&A, 504, 915 Google Scholar
Dalla Vedova, G., Millour, F., Domiciano de Souza, A., et al. 2017, A&A, 601, A118 Google Scholar
Doazan, V., Franco, M., Rusconi, L., Sedmak, G., & Stalio, R. 1983, A&A, 128, 171 Google Scholar
Ghoreyshi, M. R., Carciofi, A. C., Rmulo, L. R., et al. 2018, MNRAS, 479, 2214 CrossRefGoogle Scholar
Granada, A., Ekström, S., Georgy, C., et al. 2013, A&A, 553, A25 Google Scholar
Haberl, F. & Sturm, R. 2016, A&A, 586, A81 Google Scholar
Halonen, R. J. & Jones, C. E. 2013, ApJ, 765, 17 CrossRefGoogle Scholar
Haubois, X., Carciofi, A. C., Rivinius, T., Okazaki, A. T., & Bjorkman, J. E. 2012, ApJ, 756, 156 CrossRefGoogle Scholar
Hirata, R. 2007, in Astronomical Society of the Pacific Conference Series, Vol. 361, Active OB-Stars: Laboratories for Stellare and Circumstellar Physics, ed. Štefl, S., Owocki, S. P., & Okazaki, A. T., 267 Google Scholar
Hummel, W. 1998, A&A, 330, 243 Google Scholar
Klement, R., Carciofi, A. C., Rivinius, T., et al. 2017, A&A, 601, A74 Google Scholar
Koubský, P., Kotková, L., Votruba, V., Šlechta, M., & Dvoáková, Š. 2012, A&A, 545, A121 Google Scholar
Krtika, J., Owocki, S. P., & Meynet, G. 2011, A&A, 527, A84 Google Scholar
Meilland, A., Stee, P., Vannier, M., et al. 2007, A&A, 464, 59 Google Scholar
Panoglou, D., Carciofi, A. C., Vieira, R. G., et al. 2016, MNRAS, 461, 2616 CrossRefGoogle Scholar
Panoglou, D., Faes, D. M., Carciofi, A. C., et al. 2018, MNRAS, 473, 3039 CrossRefGoogle Scholar
Pepper, J., Pogge, R. W., DePoy, D. L., et al. 2007, PASP, 119, 923 CrossRefGoogle Scholar
Pojmanski, G. 1997, Acta Astron., 47, 467 Google Scholar
Raguzova, N. V. & Popov, S. B. 2005, Astronomical and Astrophysical Transactions, 24, 151 CrossRefGoogle Scholar
Reig, P. 2011, Ap&SS, 332, 1 Google Scholar
Reig, P., Negueruela, I., Coe, M. J., et al. 2000, MNRAS, 317, 205 CrossRefGoogle Scholar
Rmulo, L. R., Carciofi, A. C., Vieira, R. G., et al. 2018, MNRAS, 476, 3555 CrossRefGoogle Scholar
Rivinius, T., Carciofi, A. C., & Martayan, C. 2013, A&A Rev., 21, 69 Google Scholar
Rivinius, T. & Štefl, S. 2000, in Astronomical Society of the Pacific Conference Series, Vol. 214, IAU Colloq. 175: The Be Phenomenon in Early-Type Stars, ed. Smith, M. A., Henrichs, H. F., & Fabregat, J., 581 Google Scholar
Rivinius, T., Vanzi, L., Chacon, J., et al. 2012, in Astronomical Society of the Pacific Conference Series, Vol. 464, Circumstellar Dynamics at High Resolution, ed. Carciofi, A. C. & Rivinius, T., 75 Google Scholar
Secchi, A. 1867, Astronomische Nachrichten, 68, 63 CrossRefGoogle Scholar
Shokry, A., Rivinius, T., Mehner, A., et al. 2018, A&A, 609, A108 Google Scholar
Sigut, T. A. A., McGill, M. A., & Jones, C. E. 2009, ApJ, 699, 1973 CrossRefGoogle Scholar
Smith, M. A., Lopes de Oliveira, R., & Motch, C. 2016, Advances in Space Research, 58, 782 CrossRefGoogle Scholar
Udalski, A., Szymański, M. K., & Szymański, G. 2015, Acta Astron., 65, 1 Google Scholar
Underhill, A. & Doazan, V. 1982, B Stars with and without emission lines (NASA)Google Scholar
Štefl, S., Rivinius, T., Carciofi, A. C., et al. 2009, A&A, 504, 929 Google Scholar
Vieira, R. G., Carciofi, A. C., & Bjorkman, J. E. 2015, MNRAS, 454, 2107 CrossRefGoogle Scholar
Vieira, R. G., Carciofi, A. C., Bjorkman, J. E., et al. 2017, MNRAS, 464, 3071 CrossRefGoogle Scholar
Wang, L., Gies, D. R., & Peters, G. J. 2018, ApJ, 853, 156 CrossRefGoogle Scholar
Wood, K., Bjorkman, K. S., & Bjorkman, J. E. 1997, ApJ, 477, 926 CrossRefGoogle Scholar