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dc.date.accessioned 2022-07-06T16:57:37Z
dc.date.available 2022-07-06T16:57:37Z
dc.date.issued 2021-06-28
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/139050
dc.description.abstract Jets, collimated outflows of particles and fields, are observed in a wide variety of astrophysical systems, including Active Galactic Nuclei of various types, microquasars, gamma-ray bursts, and young stellar objects. Despite intensive efforts along several decades of observational and theoretical research, there are still many uncertainties and open questions related to how jets are produced and what is their composition. In this review I offer an outline of some current views on the content and basic properties of astrophysical jets. en
dc.language en es
dc.subject Jets es
dc.subject black holes es
dc.subject magnetic fields es
dc.subject accretion es
dc.title The content of astrophysical jets en
dc.type Articulo es
sedici.identifier.other doi:10.1002/asna.202113989 es
sedici.identifier.issn 0004-6337 es
sedici.identifier.issn 1521-3994 es
sedici.creator.person Romero, Gustavo Esteban es
sedici.subject.materias Astronomía es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Instituto Argentino de Radioastronomía es
sedici.subtype Preprint 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.description.peerReview peer-review es
sedici.relation.journalTitle Astronomische Nachrichten es
sedici.relation.journalVolumeAndIssue vol. 342, no. 5 es


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