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dc.contributor.authorHannikainen, D.C.
dc.contributor.authorWu, K.
dc.contributor.authorStevens, Jason
dc.contributor.authorVilhu, O.
dc.contributor.authorRodriguez, J.
dc.contributor.authorHjalmarsdotter, L.
dc.contributor.authorHunstead, R.W.
dc.identifier.citationHannikainen , D C , Wu , K , Stevens , J , Vilhu , O , Rodriguez , J , Hjalmarsdotter , L & Hunstead , R W 2006 , ' Microquasars : What do radio and X-ray observations tell us? ' , Chinese Journal of Astronomy and Astrophysics , vol. 6 , no. Supp 1 , pp. 269-278 .
dc.identifier.otherPURE: 524563
dc.identifier.otherPURE UUID: 880b75cb-2d01-4bf1-bdb8-687ec75699bd
dc.identifier.otherBibtex: urn:a33492dbcc6559a5d94c7b21915e2976
dc.identifier.otherScopus: 84900007897
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747581
dc.description.abstractMicroquasars, or X-ray binaries exhibiting radio jets, have been observed extensively at all wavelengths for the past decade or so. Primarily, they have been observed in the X-ray regimes and the radio. In this paper we review the radio and the X-ray behavior of the first two superluminal microquasars, GRS 1915+105 and GRO J1655-40. We show how GRO J1665-40 really does behave like a ``micro''-quasar based on the similarity of the radio properties between the source and quasars, and we also show some recent X-ray/γ-ray results obtained with INTEGRAL and RXTE on the notorious microquasar, GRS 1915+105.en
dc.relation.ispartofChinese Journal of Astronomy and Astrophysics
dc.titleMicroquasars : What do radio and X-ray observations tell us?en
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusNon peer reviewed
rioxxterms.typeJournal Article/Review

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