Type I x-ray bursts in GS 1826-24
Type I X-ray bursts in low-mass X-ray binaries are well understood to be due to thermonuclear flashes from accreting neutron stars. Previous work on the modeling of bursts from GS 1826-24 has had good results in reproducing the main bursting characteristics, particularly the lightcurves. We show tha...
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| Format: | Others |
| Language: | en |
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McGill University
2010
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| Online Access: | http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=95055 |