QPOs and Resonance in Accretion Disks
We review arguments suggesting that millisecond variability detected in the X-ray flux of LMXBs has its originin oscillation modes of the accretion disk. The twin high-frequency QPOs observed in microquasars seem to berelated to the twin kHz QPOs in neutron-star systems, and both phenomena are likel...
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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autori principali: | , , , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2007
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57102704 |
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