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Detection of the progenitors of Be X-ray Binaries

Published online by Cambridge University Press:  30 December 2019

Douglas Gies Open the ORCID record for Douglas Gies [Opens in a new window] ,
Luqian Wang Open the ORCID record for Luqian Wang [Opens in a new window]  and
Geraldine Peters
Douglas Gies
Affiliation:
CHARA, Dept. of Physics & Astronomy, Georgia State University, P.O. Box 5060, Atlanta, GA 30302-5060, USA emails: gies@chara.gsu.edu, lwang@chara.gsu.edu
Luqian Wang
Affiliation:
CHARA, Dept. of Physics & Astronomy, Georgia State University, P.O. Box 5060, Atlanta, GA 30302-5060, USA emails: gies@chara.gsu.edu, lwang@chara.gsu.edu
Geraldine Peters
Affiliation:
Space Sciences Center, University of Southern California, Los Angeles, CA 90089-1341, USA email: gpeters@usc.edu
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Abstract

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A recent survey of the far-ultraviolet spectra of 264 B-emission line stars has revealed 16 systems with hot companions that are the stripped down remains of a former mass donor star. Some of these will probably become Be + neutron star X-ray binaries in the future. The actual numbers of such systems may be large, because the detected systems have companions that occupy the brief and bright, He-shell burning stage of evolution.

Keywords

binaries: spectroscopicstars: emission-line Bestars: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S346: High-mass X-ray Binaries: Illuminating the Passage from Massive Binaries to Merging Compact Objects , August 2018 , pp. 143 - 145
Copyright
© International Astronomical Union 2019 

References

Chojnowski, S.D., Labadie-Bartz, J., Rivinius, T., Gies, D., Panoglou, D., Borges Fernandes, M., Wisniewski, J. P., Whelan, D. G., Mennickent, R. E., McMillan, R., Dembicky, J. M., Gray, C., Rudyk, T., Stringfellow, G. S., Lester, K., Hasselquist, S., Zharikov, S., Levenhagen, R., Souza, T., Leister, N., Stassun, K., Siverd, R. J., & Majewski, S. R. 2018 ApJ, 865, 76 CrossRefGoogle Scholar
Matson, R. A., Gies, D. R., Guo, Z., Quinn, S. N., Buchhave, L. A., Latham, D. W., Howell, S. B., & Rowe, J. F. 2015, ApJ, 806, 155 CrossRefGoogle Scholar
Mourard, D., Monnier, J. D., Meilland, A., Gies, D., Millour, F., Benisty, M., Che, X., Grundstrom, E. D., Ligi, R., Schaefer, G., Baron, F., Kraus, S., Zhao, M., Pedretti, E., Berio, P., Clausse, J. M., Nardetto, N., Perraut, K., Spang, A., Stee, P., Tallon-Bosc, I., McAlister, H., ten Brummelaar, T., Ridgway, S. T., Sturmann, J., Sturmann, L., Turner, N., & Farrington, C. 2015, A&A, 577, A51 Google Scholar
Peters, G. J., Gies, D. R., Grundstrom, E. D., & McSwain, M. V. 2008, ApJ, 686, 1280 CrossRefGoogle Scholar
Peters, G. J., Pewett, T. D., Gies, D. R., Touhami, Y. N., & Grundstrom, E. D. 2013, ApJ, 765, 2 CrossRefGoogle Scholar
Peters, G. J., Wang, L., Gies, D. R., & Grundstrom, E. D. 2016, ApJ, 828, 47 CrossRefGoogle Scholar
Pols, O. R., Cote, J., Waters, L. B. F. M., & Heise, J. 1991, A&A, 241, 419 Google Scholar
Reig, P. 2011, Ap&SS, 332, 1 Google Scholar
Rivinius, T., Carciofi, A. C., & Martayan, C. 2013, A&AR, 21, 69 Google Scholar
Schootemeijer, A., Götberg, Y., de Mink, S. E., Gies, D., & Zapartas, E. 2018, A&A, 615, A30 Google Scholar
Wang, L., Gies, D. R., & Peters, G. J. 2017, ApJ, 843, 60 CrossRefGoogle Scholar
Wang, L., Gies, D. R., & Peters, G. J. 2018, ApJ, 853, 156 CrossRefGoogle Scholar
Yudin, R. V. 2001, A&A, 368, 912 Google Scholar