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Why soft X-ray transients can remain in the low/hard state during outburst

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Meyer-Hofmeister,  E.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;
High Energy Astrophysics, MPI for Astrophysics, Max Planck Society;

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Meyer-Hofmeister, E. (2004). Why soft X-ray transients can remain in the low/hard state during outburst. Astronomy & Astrophysics, 423(1), 321-326. doi:10.1051/0004-6361:20040369.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0011-B5ED-0
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