SSSs as progenitors of the BHCs

W. Kundt

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https://doi.org/10.1...arrow_drop_down

https://doi.org/10.1007/bfb010...

Part of book or chapter of book . 2007 . Peer-reviewed

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https://dx.doi.org/10.1007/bfb...

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SSSs as progenitors of the BHCs

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Other literature type 04 Jan 2007 English Publisher:Springer Berlin Heidelberg

Authors: W. Kundt;

doi: 10.1007/bfb0102245

SSSs as progenitors of the BHCs

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Abstract

In contrast to white dwarfs, neutron stars with near companions can get surrounded by massive accretion disks when their donor stars transfer matter at a greater-than-Eddington rate for sufficiently long. When the disk gets massive, the system will successively pass through the stages of super-Eddington (SES) and/or supersoft (SSS), and end up as a black-hole candidate (BHC).

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University of Bonn
Germany

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