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Conference Paper: Inward emission in pulsar magnetosphere

TitleInward emission in pulsar magnetosphere
Authors
Dyks, J.Fra̧ckowiak, M.Słowikowska, A.Rudak, B.Zhang, Bing
KeywordsPulsars
Issue Date2005
Citation
Aip Conference Proceedings, 2005, v. 801, p. 265-271 How to Cite?
DOI: http://dx.doi.org/10.1063/1.2141878
AbstractWe discuss theoretical arguments and observational evidence for the existence of inward emission in pulsar magnetosphere. We show that the new soft components in the X-ray/UV pulse profile of the Vela pulsar can be interpreted in terms of the inward emission from the same outer magnetospheric regions that are thought to be responsible for the outward gamma-ray emission observed above 100 MeV. In the radio band, inward emission provides a way to interpret the main-pulse/interpulse anticorrelation in B1822-09 as well as the locations of emission and absorption features in the pulse profile of B0950+08. © 2005 American Institute of Physics.
Persistent Identifierhttp://hdl.handle.net/10722/361044
ISSN
0094-243X
2023 SCImago Journal Rankings: 0.152

 

DC FieldValueLanguage
dc.contributor.authorDyks, J.-
dc.contributor.authorFra̧ckowiak, M.-
dc.contributor.authorSłowikowska, A.-
dc.contributor.authorRudak, B.-
dc.contributor.authorZhang, Bing-
dc.date.accessioned2025-09-16T04:14:26Z-
dc.date.available2025-09-16T04:14:26Z-
dc.date.issued2005-
dc.identifier.citationAip Conference Proceedings, 2005, v. 801, p. 265-271-
dc.identifier.issn0094-243X-
dc.identifier.urihttp://hdl.handle.net/10722/361044-
dc.description.abstractWe discuss theoretical arguments and observational evidence for the existence of inward emission in pulsar magnetosphere. We show that the new soft components in the X-ray/UV pulse profile of the Vela pulsar can be interpreted in terms of the inward emission from the same outer magnetospheric regions that are thought to be responsible for the outward gamma-ray emission observed above 100 MeV. In the radio band, inward emission provides a way to interpret the main-pulse/interpulse anticorrelation in B1822-09 as well as the locations of emission and absorption features in the pulse profile of B0950+08. © 2005 American Institute of Physics.-
dc.languageeng-
dc.relation.ispartofAip Conference Proceedings-
dc.subjectPulsars-
dc.titleInward emission in pulsar magnetosphere-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1063/1.2141878-
dc.identifier.scopuseid_2-s2.0-33751209793-
dc.identifier.volume801-
dc.identifier.spage265-
dc.identifier.epage271-
dc.identifier.eissn1551-7616-

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