| dc.creator |
Sierpowska-Bartosik, Agnieszka |
|
| dc.creator |
Torres, Diego F. |
|
| dc.date |
2008-06-29T16:03:57Z |
|
| dc.date |
2008-06-29T16:03:57Z |
|
| dc.date |
2007-11-19 |
|
| dc.date.accessioned |
2017-01-31T02:13:34Z |
|
| dc.date.available |
2017-01-31T02:13:34Z |
|
| dc.identifier |
The Astrophysical Journal Letters 671(2): L145-L148 (2007) |
|
| dc.identifier |
0004-637X (Print) |
|
| dc.identifier |
1538-4357 (Online) |
|
| dc.identifier |
http://hdl.handle.net/10261/5431 |
|
| dc.identifier |
10.1086/525041 |
|
| dc.identifier.uri |
http://dspace.mediu.edu.my:8181/xmlui/handle/10261/5431 |
|
| dc.description |
4 pages.-- Printed version published on Dec 20, 2007. |
|
| dc.description |
Under the assumption that LS 5039 is a system composed of a pulsar rotating around an O6.5 V star in a ~3.9 day orbit, we present the results of a theoretical modeling of the high-energy phenomenology observed by the High Energy Stereoscopy Array (H.E.S.S.). This model (including a detailed account of the system geometry, Klein-Nishina inverse Compton scattering, γ-γ absorption, and cascading) is able to describe well the rich observed phenomenology found in the system at all timescales, both flux- and spectrum-wise. |
|
| dc.description |
We acknowledge support by grants AYA 2006-00530 and CSIC-PIE 200750I029. |
|
| dc.description |
Peer reviewed |
|
| dc.format |
409787 bytes |
|
| dc.format |
application/pdf |
|
| dc.language |
eng |
|
| dc.publisher |
American Astronomical Society |
|
| dc.publisher |
University of Chicago Press |
|
| dc.relation |
http://dx.doi.org/10.1086/525041 |
|
| dc.rights |
openAccess |
|
| dc.subject |
X-ray binaries (individual LS 5039) |
|
| dc.subject |
γ-rays: observations |
|
| dc.subject |
γ-rays: theory |
|
| dc.subject |
High Energy Stereoscopy Array (H.E.S.S.) Telescope |
|
| dc.title |
Pulsar model of the high energy phenomenology of LS 5039 |
|
| dc.type |
Artículo |
|