Hostname: page-component-cd9895bd7-q99xh Total loading time: 0 Render date: 2024-12-24T16:42:27.153Z Has data issue: false hasContentIssue false
  • English
  • Français

Links Between Z Sources and Atoll Sources

Published online by Cambridge University Press:  21 February 2013

Joan Jing Wang  and
Hsiang-Kuang Chang
Joan Jing Wang
Affiliation:
Institute of Astronomy, National Tsing Hua University, Hsinchu 30013, Taiwan email: [email protected]
Hsiang-Kuang Chang
Affiliation:
Institute of Astronomy, National Tsing Hua University, Hsinchu 30013, Taiwan email: [email protected] Department of Physics, National Tsing Hua University, Hsinchu 30013, Taiwan email: [email protected]
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.

It is known that the Z and atoll sources are two typical types of neutron-star sources in low mass X-ray binaries (LMXBs), which present very different Q-ν relations of lower kHz QPOs. We propose that the Z and atoll sources are two different phases in the evolutionary track of neutron star in LMXBs, instead of two types of distinct sources.

Keywords

LMXBsZ sourceatoll source
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S290: Feeding Compact Objects: Accretion on All Scales , August 2012 , pp. 331 - 332
Copyright
Copyright © International Astronomical Union 2013

References

Camenzind, M. 2007, Compact Objects in Astrophysics: White Dwarfs, Neutron Stars, and Black Holes. Springer-Verlag, BerlinGoogle Scholar
Ding, G. Q., Zhang, S. N., Wang, N., Qu, J. L., & Yan, S. P. 2011, AJ, 142, 34CrossRefGoogle Scholar
Frank, J., King, A., & Raine, D. 2002, Accretion Power in Astrophysics (Cambridge, UK: Cambridge University Press)CrossRefGoogle Scholar
Gierliński, M. & Done, C. 2002, MNRAS, 331, L47CrossRefGoogle Scholar
Hasinger, G. & van der Klis, M. 1989, A&A, 225, 79Google Scholar
Homan, J., Wijnands, R., Rupen, M. P., Fender, R., Hjellming, R. M., di Salvo, T., & van der Klis, M. 2004, A&A, 418, 255Google Scholar
Liu, Q. Z., van Paradijs, J., & van den Heuvel, E. P. J. 2007, A&A, 469, 807Google Scholar
Paczyńsky, B. & Wiita, P. J. 1980, A&A, 88, 23Google Scholar
Romanova, M. M., Kulkarni, A. K., & Lovelace, R. V. E. 2007 (astroph/0711.0418)Google Scholar
Schnerr, R. S., Reerink, T., van der Klis, M., Homan, J., Méndez, M., Fender, R. P., & Kuulkers, E. 2003, A&A, 406, 221Google Scholar
Wang, J., Chang, H. K., Zhang, C. M.et al. 2012, Astrophysics and Space Science, 342, 357CrossRefGoogle Scholar
Zhang, C. M. & Kojima, Y. 2006, MNRAS, 366, 137Google Scholar