Laboratory study of stationary accretion shock relevant to astrophysical systems

Author:

Mabey P.,Albertazzi B.,Falize E.,Michel Th.,Rigon G.ORCID,Van Box Som L.,Pelka A.,Brack F.-E.ORCID,Kroll F.ORCID,Filippov E.ORCID,Gregori G.,Kuramitsu Y.,Lamb D. Q.,Li C.,Ozaki N.,Pikuz S.ORCID,Sakawa Y.,Tzeferacos P.,Koenig M.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Reference46 articles.

1. Frank, J., King, A. & Raine, D. Accretion power in astrophysics. (Cambridge university press, 2002).

2. Ghosh, P. & Lamb, F. K. Accretion by rotating magnetic neutron stars. ii-radial and vertical structure of the transition zone in disk accretion. The Astrophysical Journal 232, 259–276 (1979).

3. Ghosh, P. & Lamb, F. K. Accretion by rotating magnetic neutron stars. iii. accretion torques and period changes in pulsating x-ray sources’. Accretion: A Collection Of Inuential Papers 5, 300 (1989).

4. Koenigl, A. Disk accretion onto magnetic t tauri stars. The Astrophysical Journal 370, L39–L43 (1991).

5. Bouvier, J., Alencar, S. H. P., Harries, T. J., Johns-Krull, C. M. & Romanova, M. M. Magnetospheric accretion in classical t tauri stars. arXiv preprint astro-ph/0603498 (2006).

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