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dc.date.accessioned 2022-12-07T17:29:06Z
dc.date.available 2022-12-07T17:29:06Z
dc.date.issued 2011-06-06
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/147029
dc.description.abstract T Tauri stars are young, low mass, pre-main sequence stars surrounded by an accretion disk. These objects present strong magnetic activity and powerful magnetic reconnection events. Strong shocks are likely produced in the stellar magnetosphere by such events and charged particles accelerated up to relativistic energies. We present a simple model for the non-thermal radiation generated by high-energy particles in T Tauri stars. We discuss whether this emission is detectable at high energies with the available gamma-ray telescopes. en
dc.language es es
dc.title High-energy radiation from T Tauri stars en
dc.type Articulo es
sedici.identifier.other doi:10.22323/1.123.0173 es
sedici.creator.person Romero, Gustavo Esteban es
sedici.creator.person Valle, María Victoria del es
sedici.creator.person Martí, Josep es
sedici.creator.person Luque Escamilla, Pedro es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Instituto Argentino de Radioastronomía es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution 4.0 International (CC BY 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by/4.0/
sedici.relation.event 25th Texas Symposium on Relativistic Astrophysics (Texas, 2010) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Proceedings of Science es
sedici.relation.journalVolumeAndIssue vol. 123 es


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Creative Commons Attribution 4.0 International (CC BY 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution 4.0 International (CC BY 4.0)