| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10694249 | Advances in Space Research | 2015 | 9 Pages |
Abstract
The difference between the cumulative luminosity distributions of classical SgXBs and SFXTs is interpreted in terms of accretion from a structured wind in the former sources and the presence of magnetic/centrifugal gates or a quasi-spherical settling accretion regime in the latter.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
E. Bozzo, P. Romano, L. Ducci, F. Bernardini, M. Falanga,