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dc.date.accessioned 2020-06-22T16:54:49Z
dc.date.available 2020-06-22T16:54:49Z
dc.date.issued 2010-05
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/98761
dc.description.abstract Some early-type stars are detectable radio emitters; their spectra can present both thermal and non-thermal contributions. Here I review the public radio data on OB stars, focusing on the non-thermal sources. The analysis of the statistical results gives rise to many open questions that are expected to be addressed, at least in part, with the upgrades of current radio telescopes and the upcoming new generation instruments. en
dc.format.extent 111-121 es
dc.language en es
dc.subject Radio continuum es
dc.subject Nonthermal mechanisms es
dc.subject Early-type stars es
dc.subject Radiation mechanisms es
dc.title Non-thermal radio emission from OB stars: an observer’s view en
dc.type Articulo es
sedici.identifier.uri https://ri.conicet.gov.ar/11336/6324 es
sedici.identifier.uri http://www.aspbooks.org/a/volumes/article_details/?paper_id=31092 es
sedici.identifier.uri https://arxiv.org/abs/0904.0533v1 es
sedici.identifier.other arXiv:0904.0533v1 es
sedici.identifier.other hdl:11336/6324 es
sedici.identifier.issn 0004-6280 es
sedici.creator.person Benaglia, Paula es
sedici.subject.materias Astronomía 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-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.event High Energy Phenomena in Massive Stars (University of Jaén, Spain, 2010) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle ASP Conference Series es
sedici.relation.journalVolumeAndIssue vol. 422 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)