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Realistic Models for Donors in Ultracompact Binaries

Published online by Cambridge University Press:  22 February 2018

C. J. Deloye  and
L. Bildsten
C. J. Deloye
Affiliation:
Dept. of Physics, UCSB
L. Bildsten
Affiliation:
Dept. of Physics, UCSB KITP, UCSB

Abstract

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We present the first realistic set of arbitrarily degenerate stellar models appropriate for donors in ultracompact binaries. The mass-radius M-R relations for these objects are parameterized by the donor's entropy and composition. We highlight how this fact can affect our understanding on the current configuration of ultracompact binaries today and their potential evolutionary tracks.

Resumen

Resumen

Presentamos el primer conjunto realista de modelos estelares arbitrariamente degenerados, apropiados para donadores en binarias ultracompactas. Las relaciones masa - radio, M-R, de estos objetos son parametrizadas por la entropía y la composición del donador. Enfatizamos que nuestra comprensión de la configuración actual de binarias ultracompactas y sus potenciales trazas evolutivas pueden estar afectadas por este hecho.

Keywords

BinariesClose — White Dwarfs — X-RaysBinaries
Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 95 - 96
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

Bildsten, L. 2002, ApJ, 577, L27 Google Scholar
Deloye, ?. J. & Bildsten, L., 2003, ApJ, in press.Google Scholar
Fedorova, A. V. & Ergma, E. V. 1989, Ap&SS, 151, 125 Google Scholar
Galloway, D. K., Chakrabarty, D., Morgan, E. H., Remillard, R. A. 2002, ApJ, 576, L137 Google Scholar
Markwardt, ?. ?., Swank, J. H., Strohymayer, T. E., in 't Zand, J. J. M., & Marshall, F. E. 2002, ApJ, 575, L21 CrossRefGoogle Scholar
Markwardt, ?. ?., Smith, E., & Swank, J. H., 2003a, IAUC Circ. No. 8080Google Scholar
Markwardt, ?. ?., Juda, M., & Swank, J. H., 2003b, IAUC Circ. No. 8095Google Scholar
Nelson, L. A., Rappaport, S. A., Joss, P. C. 1986, ApJ, 304, 231 Google Scholar
Nelson, L. A. & Rappaport, S. A., 2003, ApJ, submitted, astro-ph/0304374Google Scholar
Podsiadlowski, Ph., Rappaport, S., & Pfahl, E. D. 2002, ApJ, 565, 1107 Google Scholar
Rappaport, S., Joss, P.C., & Webbink, R. F. 1982, ApJ, 254, 616 CrossRefGoogle Scholar
Salaris, M., García-Berro, E., Hernanz, M., Isern, J., & Saumon, D. 2000, ApJ, 544, 1036 Google Scholar
Serenelli, A. M., Althaus, L. G., Rohrmann, R. D., & Benvenuto, O. G. 2001, MNRAS, 325, 607 CrossRefGoogle Scholar