Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-14T09:45:53.036Z Has data issue: false hasContentIssue false
  • English
  • Français

Evolution of binaries with compact objects in globular clusters

Published online by Cambridge University Press:  07 March 2016

Natalia Ivanova
Natalia Ivanova*
Affiliation:
Dept. of Physics, University of Alberta, 11322-89 Ave, Edmonton, AB, T6G 2E7, Canada email: nata.ivanova@ualberta.ca
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.

Dynamical interactions that take place between objects in dense stellar systems lead to frequent formation of exotic stellar objects, unusual binaries, and systems of higher multiplicity. They are most important for the formation of binaries with neutron stars and black holes, which are usually observationally revealed in mass-transferring binaries. Here we review the current understanding of compact object's retention, of the metallicity dependence on the formation of low-mass X-ray binaries with neutron stars, and how mass-transferring binaries with a black hole and a white dwarf can be formed. We discuss as well one old unsolved puzzle and two new puzzles posed by recent observations: what descendants do ultra-compact X-ray binaries produce, how are very compact triples formed, and how can black hole low-mass X-ray binaries acquire non-degenerate companions?

Keywords

binaries : closeglobular clusters: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S312: Star Clusters and Black Holes in Galaxies across Cosmic Time , August 2014 , pp. 203 - 212
Copyright
Copyright © International Astronomical Union 2016 

References

Altamirano, D.et al., 2010, ApJL, 712, L58Google Scholar
Anderson, S. F.et al., 1997, ApJL, 482, L69Google Scholar
Archibald, A. M.et al., 2009, Science, 324, 1411CrossRefGoogle Scholar
Bagchi, M., Lorimer, D. R., & Chennamangalam, J., 2011, MNRAS, 418, 477Google Scholar
Bahramian, A.et al., 2014, ApJ, 780, 127CrossRefGoogle Scholar
Bahramian, A., Heinke, C. O., Sivakoff, G. R., & Gladstone, J. C., 2013, ApJ, 766, 136Google Scholar
Bailes, M.et al., 2011, Science, 333, 1717Google Scholar
Bałucińska-Church, M., Church, M. J., & Smale, A. P., 2004, MNRAS, 347, 334CrossRefGoogle Scholar
Belczynski, K., Sadowski, A., Rasio, F. A., & Bulik, T., 2006, ApJ, 650, 303Google Scholar
Bellazzini, M.et al., 1995, ApJ, 439, 687Google Scholar
Benvenuto, O. G., De Vito, M. A., & Horvath, J. E., 2012, ApJL, 753, L33Google Scholar
Bhattacharya, D. & van den Heuvel, E. P. J., 1991, Phys.Rep., 203, 1Google Scholar
Bildsten, L. & Deloye, C. J., 2004, ApJL, 607, L119Google Scholar
Blaes, O., Lee, M. H., & Socrates, A., 2002, ApJ, 578, 775Google Scholar
Bordas, P.et al., 2010, The Astronomer's Telegram, 2919, 1Google Scholar
Bozzo, E.et al., 2011, A&A, 535, L1Google Scholar
Brandt, N. & Podsiadlowski, P., 1995, MNRAS, 274, 461Google Scholar
Brodie, J. P. & Strader, J., 2006, ARAA, 44, 193Google Scholar
Cartwright, T. F.et al., 2013, ApJ, 768, 183Google Scholar
Castro-Tirado, A. J., Brandt, S., & Lund, N., 1992, IAU circular, 5590, 2Google Scholar
Chomiuk, L.et al., 2013, ApJ, 777, 69CrossRefGoogle Scholar
Chou, Y. & Grindlay, J. E., 2001, ApJ, 563, 934Google Scholar
Deegan, P., Combet, C., & Wynn, G. A., 2009, MNRAS, 400, 1337Google Scholar
Deloye, C. J., 2008, in AIP Conference Series, Vol. 983, 40 Years of Pulsars, Bassa, C., Wang, Z., Cumming, A., Kaspi, V. M., eds., pp. 501–509Google Scholar
Deloye, C. J. & Bildsten, L., 2003, ApJ, 598, 1217Google Scholar
Dessart, L.et al., 2006, ApJ, 644, 1063CrossRefGoogle Scholar
Downing, J. M. B., Benacquista, M. J., Giersz, M., & Spurzem, R., 2010, MNRAS, 407, 1946Google Scholar
Drukier, G. A., 1996, MNRAS, 280, 498Google Scholar
Eckert, D.et al., 2013, The Astronomer's Telegram, 4925, 1Google Scholar
Eggleton, P., 2006, Evolutionary Processes in Binary and Multiple StarsGoogle Scholar
Eggleton, P. P. & Kisseleva-Eggleton, L., 2006, Ap&SS, 304, 75Google Scholar
Engel, M. C.et al., 2012, ApJ, 747, 119Google Scholar
Fabrycky, D. & Tremaine, S., 2007, ApJ, 669, 1298Google Scholar
Ford, E. B., Kozinsky, B., & Rasio, F. A., 2000, ApJ, 535, 385Google Scholar
Fragos, T.et al., 2008, ApJ, 683, 346CrossRefGoogle Scholar
Fragos, T.et al., 2009, ApJL, 702, L143CrossRefGoogle Scholar
Fregeau, J. M., Cheung, P., Portegies Zwart, S. F., & Rasio, F. A., 2004, MNRAS, 352, 1Google Scholar
Giacconi, R.et al., 1974, ApJ Supp, 27, 37Google Scholar
Grindlay, J. E., 1984, Advances in Space Research, 3, 19Google Scholar
Grindlay, J. E., 1993, in ASP Conference Series, Vol. 48, The Globular Cluster-Galaxy Connection, Smith, G. H., Brodie, J. P., eds., p. 156Google Scholar
Guainazzi, M., Parmar, A. N., & Oosterbroek, T., 1999, A&A, 349, 819Google Scholar
Heinke, C. O.et al., 2010, ApJ, 714, 894Google Scholar
Heinke, C. O.et al., 2013, ApJ, 768, 184Google Scholar
Hobbs, G., Lorimer, D. R., Lyne, A. G., & Kramer, M., 2005, MNRAS, 360, 974Google Scholar
Humphrey, P. J. & Buote, D. A., 2008, ApJ, 689, 983Google Scholar
Ivanova, N., 2006, ApJ, 636, 979Google Scholar
Ivanova, N., 2008, in Multiple Stars Across the H-R Diagram, Hubrig, S., Petr-Gotzens, M., Tokovinin, A., eds., p. 101CrossRefGoogle Scholar
Ivanova, N.et al., 2010, ApJ, 717, 948Google Scholar
Ivanova, N.et al., 2012, ApJL, 760, L24Google Scholar
Ivanova, N., Heinke, C. O., & Rasio, F. A., 2008a, in AIP Conference Series, Vol. 983, 40 Years of Pulsars, Bassa, C., Wang, Z., Cumming, A., Kaspi, V. M., eds., pp. 442–447Google Scholar
Ivanova, N.et al., 2008b, MNRAS, 386, 553Google Scholar
Ivanova, N.et al., 2013, Astronomy and Astrophysics Review, 21, 59Google Scholar
Ivanova, N.et al., 2005, ApJL, 621, L109CrossRefGoogle Scholar
Kalogera, V., King, A. R., & Rasio, F. A., 2004, ApJL, 601, L171Google Scholar
Kim, D.-W.et al., 2013, ApJ, 764, 98Google Scholar
Kim, E.et al., 2006, ApJ, 647, 276CrossRefGoogle Scholar
Kitaura, F. S., Janka, H.-T., & Hillebrandt, W., 2006, A&A, 450, 345Google Scholar
Knigge, C., Baraffe, I., & Patterson, J., 2011, ApJ Supp, 194, 28Google Scholar
Kozai, Y., 1962, AJ, 67, 591Google Scholar
Kroupa, P., 2002, Science, 295, 82Google Scholar
Kulkarni, S. R., Hut, P., & McMillan, S., 1993, Nature, 364, 421Google Scholar
Kundu, A., Maccarone, T. J., & Zepf, S. E., 2002, ApJL, 574, L5Google Scholar
Lombardi, J. C. Jr.et al., 2006, ApJ, 640, 441Google Scholar
Maccarone, T. J., Kundu, A., Zepf, S. E., & Rhode, K. L., 2010, MNRAS, 409, L84Google Scholar
Miyaji, S., Nomoto, K., Yokoi, K., & Sugimoto, D., 1980, PASJ, 32, 303Google Scholar
Morscher, M.et al., 2014, ArXiv e-printsGoogle Scholar
Morscher, M., Umbreit, S., Farr, W. M., & Rasio, F. A., 2013, ApJL, 763, L15Google Scholar
Nomoto, K., 1984, ApJ, 277, 791Google Scholar
O'Leary, R. M.et al., 2006, ApJ, 637, 937Google Scholar
Paolillo, M.et al., 2011, ApJ, 736, 90Google Scholar
Papitto, A.et al., 2013, Nature, 501, 517Google Scholar
Peuten, M., Brockamp, M., Küpper, A. H. W., & Kroupa, P., 2014, ApJ, 795, 116Google Scholar
Pfahl, E., Rappaport, S., & Podsiadlowski, P., 2002, ApJ, 573, 283CrossRefGoogle Scholar
Pletsch, H. J.et al., 2012, Science, 338, 1314Google Scholar
Podsiadlowski, P.et al., 2004, ApJ, 612, 1044Google Scholar
Pols, O. R., Tout, C. A., Eggleton, P. P., & Han, Z., 1995, MNRAS, 274, 964Google Scholar
Pooley, D.et al., 2003, ApJL, 591, L131Google Scholar
Portegies Zwart, S. F., & Meinen, A. T., 1993, A&A, 280, 174Google Scholar
Prodan, S. & Murray, N., 2012, ApJ, 747, 4Google Scholar
Prodan, S. & Murray, N., 2014, ArXiv e-printsGoogle Scholar
Rappaport, S., Ma, C. P., Joss, P. C., & Nelson, L. A., 1987, ApJ, 322, 842Google Scholar
Romani, R. W.et al., 2012, ApJL, 760, L36CrossRefGoogle Scholar
Sarazin, C. L.et al., 2003, ApJ, 595, 743Google Scholar
Sivakoff, G. R.et al., 2007, ApJ, 660, 1246Google Scholar
Spitzer, L. Jr., 1969, ApJL, 158, L139Google Scholar
Stella, L., Priedhorsky, W., & White, N. E., 1987, ApJL, 312, L17Google Scholar
Strader, J.et al., 2012, Nature, 490, 71Google Scholar
Tauris, T. M. & van den Heuvel, E. P. J., 2006, Formation and evolution of compact stellar X-ray sourcesCrossRefGoogle Scholar
Testa, V.et al., 2012, A&A, 547, A28Google Scholar
Timmes, F. X. & Woosley, S. E., 1992, ApJ, 396, 649Google Scholar
Tominaga, N., Blinnikov, S. I., & Nomoto, K., 2013, ApJL, 771, L12Google Scholar
van der Klis, M.et al., 1993, A&A, 279, L21Google Scholar
van Haaften, L. M., Nelemans, G., Voss, R., & Jonker, P. G., 2012a, A&A, 541, A22Google Scholar
van Haaften, L. M., Voss, R., & Nelemans, G., 2012b, A&A, 543, A121Google Scholar
Vanderbeke, J.et al., 2014a, MNRAS, 437, 1725Google Scholar
Vanderbeke, J.et al., 2014b, MNRAS, 437, 1734Google Scholar
Verbunt, F., 1987, ApJL, 312, L23Google Scholar
Verbunt, F., 1993, ARAA, 31, 93Google Scholar
Verbunt, F. & Hut, P., 1987, in IAU Symposium, Vol. 125, The Origin and Evolution of Neutron Stars, Helfand, D. J., Huang, J.-H., eds., p. 187Google Scholar
Verbunt, F. & Lewin, W. H. G., 2006, Globular cluster X-ray sources, Lewin, W. H. G., van der Klis, M., eds., pp. 341–379Google Scholar
Verbunt, F. & van den Heuvel, E. P. J., 1995, X-ray Binaries, 457Google Scholar
Wijnands, R. & van der Klis, M., 1998, Nature, 394, 344Google Scholar
Zahn, J.-P., 2008, in EAS Publications Series, Vol. 29, EAS Publications Series, Goupil, M.-J., Zahn, J.-P., eds., pp. 67–90Google Scholar
Zepf, S. E.et al., 2008, ApJL, 683, L139Google Scholar
Zurek, D. R.et al., 2009, ApJ, 699, 1113Google Scholar