Dead discs, unstable discs and the stars they surround
Strong stellar magnetic fields significantly alter the behaviour of surrounding accretion discs. Recent work has demonstrated that at low accretion rates a large amount of mass can remain confined in the disc, contrary to the standard assumption that the magnetic field will expel the disc in an outf...
| Հիմնական հեղինակ: | |
|---|---|
| Ձևաչափ: | Հոդված |
| Լեզու: | English |
| Հրապարակվել է: |
EDP Sciences
2014-01-01
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| Շարք: | EPJ Web of Conferences |
| Առցանց հասանելիություն: | http://dx.doi.org/10.1051/epjconf/20136401003 |