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MOCCA-SURVEY Database I: Dissolution of tidally filling star clusters harboring black hole subsystem

Published online by Cambridge University Press:  11 March 2020

Mirek Giersz
Affiliation:
Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, Warsaw, Poland email: mig@camk.edu.pl
Abbas Askar
Affiliation:
Lund Observatory, Department of Astronomy, and Theoretical Physics, Lund University, Box 43, SE-221 00 Lund, Sweden email: askar@astro.lu.se
Long Wang
Affiliation:
Helmholtz-Institut für Strahlen- und Kernphysik, University of Bonn, Nussallee 14-16, D-53115 Bonn, Germany Argelander Institut Für Astronomie, Auf Dem Hügel 71, 53121, Bonn, Germany RIKEN Center for Computational Science, 7-1-26 Minatojima-minami-machi, Chuo-ku, Kobe, Hyogo 650-0047, Japan email: longwang.astro@live.com
Arkadiusz Hypki
Affiliation:
Astronomical Observatory Institute, Faculty of Physics, A. Mickiewicz University, Słoneczna 36, 60-286 Poznań, Poland email: ahypki@amu.edu.pl
Agostino Leveque
Affiliation:
Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, Warsaw, Poland email: mig@camk.edu.pl
Rainer Spurzem
Affiliation:
National Astronomical Observatories and Key Laboratory for Computational Astrophysics, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, China Astronomisches Rechen-Institut, Zentrum für Astronomie, University of Heidelberg, Mönchhofstrasse 12-14, D-69120 Heidelberg, Germany Kavli Institute for Astronomy and Astrophysics, Peking University, Yi He Yuan Lu 5, HaiDian District, Beijing 100871, China email: spurzem@ari.uni-heidelberg.de
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Abstract

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We investigate the dissolution process of star clusters embedded in an external tidal field and harboring a subsystem of stellar-mass black hole. For this purpose we analyzed the MOCCA models of real star clusters contained in the Mocca Survey Database I. We showed that the presence of a stellar-mass black hole subsystem in tidally filling star cluster can lead to abrupt cluster dissolution connected with the loss of cluster dynamical equilibrium. Such cluster dissolution can be regarded as a third type of cluster dissolution mechanism. We additionally argue that such a mechanism should also work for tidally under-filling clusters with a top-heavy initial mass function.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

References

Askar, A., Szkudlarek, M., Gondek-Rosińska, D., Giersz, M., & Bulik, T. 2017, MNRAS 464, L36CrossRefGoogle Scholar
Banerjee, S. & Kroupa, P. 2011, ApJ 741, L12CrossRefGoogle Scholar
Baumgardt, H. & Makino, J. 2003, MNRAS 340, 227CrossRefGoogle Scholar
Belczynski, K., Kalogera, V. & Bulik, T. 2002, ApJ 572, 407CrossRefGoogle Scholar
Breen, P. G. & Heggie, D. C. 2013, MNRAS 432, 2779CrossRefGoogle Scholar
Chernoff, D. F. & Weinberg, M. D. 1990, ApJ 351, 121CrossRefGoogle Scholar
Contenta, F., Varri, A. L., & Heggie, D. C. 2015, MNRAS 449, L100CrossRefGoogle Scholar
Fukushige, T. & Heggie, D. C. 1995, MNRAS 276, 206Google Scholar
Giersz, M., Heggie, D. C., Hurley, J. R., & Hypki, A. 2013, MNRAS 431, 2184CrossRefGoogle Scholar
Giersz, M., Askar, A., Wang, L., Hypki, A., Laveque, A., & Spurzem, R. 2019, MNRAS 487, 2417CrossRefGoogle Scholar
Gnedin, O. Y. & Ostriker, J. P. 1997, ApJ 474, 223CrossRefGoogle Scholar
Hypki, A. & Giersz, M. 2013, MNRAS 429, 1221CrossRefGoogle Scholar
Tanikawa, A. & Fukushige, T. 2009, PASJ 61, 721CrossRefGoogle Scholar
Wang, L., Spurzem, R., Aarseth, S., Nitadori, K., Berczik, P., Kouwenhoven, M. B. N., & Naab, T. 2015, MNRAS 450, 4070CrossRefGoogle Scholar
Whitehead, A. J., McMillan, S. L. W., Vesperini, E., & Portegies Zwart, S. 2013, ApJ 778, 118CrossRefGoogle Scholar