dc.creator | Romero, Gustavo Esteban | |
dc.creator | Orellana, Mariana Dominga | |
dc.creator | Okazaki, A.T. | |
dc.creator | Owocki, S. P. | |
dc.date.accessioned | 2017-11-08T14:39:51Z | |
dc.date.accessioned | 2018-11-06T12:23:56Z | |
dc.date.available | 2017-11-08T14:39:51Z | |
dc.date.available | 2018-11-06T12:23:56Z | |
dc.date.created | 2017-11-08T14:39:51Z | |
dc.date.issued | 2008-09 | |
dc.identifier | Romero, Gustavo Esteban; Orellana, Mariana Dominga; Okazaki, A.T.; Owocki, S. P.; LS I+61 303: microquasar or not microquasar?
; World Scientific; International Journal of Modern Physics D; 17; 10; 9-2008; 1875-1881 | |
dc.identifier | 0218-2718 | |
dc.identifier | http://hdl.handle.net/11336/27815 | |
dc.identifier | 1793-6594 | |
dc.identifier | CONICET Digital | |
dc.identifier | CONICET | |
dc.identifier.uri | http://repositorioslatinoamericanos.uchile.cl/handle/2250/1866098 | |
dc.description.abstract | LS I +61 303 is a puzzling object detected from radio up to high-energy gamma-rays. Variability has recently been observed in its high-energy emission. The object is a binary system, with a compact object and a Be star as primary. The nature of the secondary and the origin of the gamma-ray emission are not clearly established at present. Recent VLBA radio data have been used to claim that the system is a Be/neutron star colliding wind binary, instead of a microquasar. We review the main views on the nature of LS I +61 303 and present results of 3D SPH simulations that can shed some light on the nature of the system. Our results support an accretion powered source, compatible with a microquasar interpretation. | |
dc.language | eng | |
dc.publisher | World Scientific | |
dc.relation | info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1142/S0218271808013510 | |
dc.relation | info:eu-repo/semantics/altIdentifier/url/http://www.worldscientific.com/doi/abs/10.1142/S0218271808013510 | |
dc.rights | https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ | |
dc.rights | info:eu-repo/semantics/openAccess | |
dc.subject | X ray binaries | |
dc.subject | Gamma rays | |
dc.subject | LS I +61 303 (estrella) | |
dc.title | LS I+61 303: microquasar or not microquasar? | |
dc.type | Artículos de revistas | |
dc.type | Artículos de revistas | |
dc.type | Artículos de revistas | |