A magnetic explanation for the rapid burster |
| |
| Authors: | J. Kuijpers M. Kuperus |
| |
| Affiliation: | (1) Sterrekundig Instituut, Universiteit Utrecht, P.O. Box 80 000, 3508 TA Utrecht;(2) CHEAF, P.O. Box 41882, 1009 DB Amsterdam;(3) Discipline Natuurkunde, Universiteit Nijmegen, Toernooiveld 1, 6525 ED Nijmegen |
| |
| Abstract: | The observations of X-ray Type II bursts from the low-mass X-ray binary MXB 1730-335 can be explained by a particular form of magnetic gating in the presence of steady external accretion. The requirements are a strong magnetic field of the neutron star (7×1011–2×1012 gauss at the surface), rotational symmetry and alignment of the field axis with the axis of a steadily accreting disk to within 6°. |
| |
| Keywords: | X-ray binary MXB 1730-335 mhd relaxation filament |
| 本文献已被 SpringerLink 等数据库收录！ |
|
