Remember Me
Or use your Academic/Social account:


Or use your Academic/Social account:


You have just completed your registration at OpenAire.

Before you can login to the site, you will need to activate your account. An e-mail will be sent to you with the proper instructions.


Please note that this site is currently undergoing Beta testing.
Any new content you create is not guaranteed to be present to the final version of the site upon release.

Thank you for your patience,
OpenAire Dev Team.

Close This Message


Verify Password:
Verify E-mail:
*All Fields Are Required.
Please Verify You Are Human:
fbtwitterlinkedinvimeoflicker grey 14rssslideshare1
Wang, Jiu-Zhou; Wang, Ding-Xiong; Huang, Chang-Yin (2013)
Languages: English
Types: Preprint
Subjects: Astrophysics - High Energy Astrophysical Phenomena

Classified by OpenAIRE into

arxiv: Astrophysics::High Energy Astrophysical Phenomena
A disk-corona model for fitting low/hard (LH) state of associated steady jet of black hole X-ray binaries (BHXBs) is proposed based on the large-scale magnetic field configuration of the coexistence of the Blandford-Znajek (BZ) and Blandford-Payne (BP) processes,where the magnetic field configuration for the BP process is determined by the requirement of energy conversion from Poynting energy flux into kinetic energy flux in the jet. It is found that corona current is crucial to guarantee the consistency of the jet launching from accretion disk. The relative importance of the BZ to BP processes in powering jets from black hole accretion disk is discussed, and the LH state of several BHXBs is fitted based on our model.In addition, we suggest that magnetic field configuration could be regarded as the second parameter for governing the state transition of BHXBs.
  • The results below are discovered through our pilot algorithms. Let us know how we are doing!

    • Belloni, T. M. 2004, Nucl. Phys. B, 132, 337
    • Belloni, T. M. 2006, AdSpR, 38, 2801
    • Belloni, T. M. 2010, The Jet Paradigm, Lecture Notes in Physics, Vol. 794, Springer-Verlag Berlin Heidelberg, p. 53
    • Belloni, T. M., Motta, S. E., & Munoz-Darias, T. 2011, BASI, 39, 409
    • Bisnovatyi-Kogan, G. S., & Ruzmaikin, A. A. 1976, Ap&SS, 42, 401
    • Blandford, R. D., & Begelman, M. C. 1999, MNRAS, 303, L1
    • Blandford, R. D., & Payne, D. G. 1982, MNRAS, 199, 883 (BP82)
    • Blandford, R. D., & Znajek, R. L. 1977, MNRAS, 179, 433
    • Cao, X. W. 2002, MNRAS, 332, 999 (C02)
    • Contopoulos, J. 1995, ApJ, 450, 616
    • Contopoulos, I., & Kazanas, D. 1998, ApJ, 508, 859
    • De Villiers, J. P., Hawley, J. F., Krolik, J. H. & Hirose, S., 2005, ApJ, 620, 878 Doeleman, et al. 2012, Science, 338, 355
    • Done, C. 2002, Royal Society of London Philosophical Transactions Series A, 360, 1967 Done, C. 2010, arXiv:1008.2287
    • Done, C., Gierlinski, M., & Kubota, A. 2007, A&AR., 15, 1
    • Esin, A. A., McClintock, J. E., & Narayan, R. 1997, ApJ, 489, 865
    • Esin, A. A., et al. 1998, ApJ, 505, 854
    • Esin, A. A., et al. 2001, ApJ, 555, 483
    • Fender, R., & Belloni, T. 2012, Science, 337, 540
    • Fender, R. P., Belloni, T. M., & Gallo, E. 2004, MNRAS, 355, 1105 (FBG04) Fender, R. P., Gallo, E., & Jonker, P. 2003, MNRAS, 343, L99
    • Fender, R. P., Gallo, E., & Rusell, D. 2010, MNRAS, 406, 1425 (FGR10)
    • Fender, R. P., Homan, J., & Belloni, T. M. 2009, MNRAS, 396, 1370
    • Gan, Z.-M., Wang, D.-X., & Lei, W.-H. 2009, MNRAS, 394, 2310 (GWL09) Ghosh, P., & Abramowicz, M. A. 1997, MNRAS, 292, 887
  • No related research data.
  • No similar publications.

Share - Bookmark

Cite this article

Collected from