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dc.contributor.authorTakami, M.
dc.contributor.authorChrysostomou, A.
dc.contributor.authorBailey, J.
dc.contributor.authorGledhill, T.
dc.contributor.authorTamura, M.
dc.contributor.authorTerada, H.
dc.identifier.citationTakami , M , Chrysostomou , A , Bailey , J , Gledhill , T , Tamura , M & Terada , H 2003 , ' Hα and Hel emission in the jets of pre-main sequence stars : implications for the heating mechanisms ' , Astrophysics and Space Science , vol. 287 , no. 1-4 , pp. 143-146 .
dc.identifier.otherPURE: 181888
dc.identifier.otherPURE UUID: 6d377d9d-7f72-4a89-b861-1920fcd0644d
dc.identifier.otherdspace: 2299/5329
dc.identifier.otherScopus: 10044230315
dc.identifier.otherORCID: /0000-0002-2859-4600/work/30779783
dc.descriptionThe original publication is available at Copyright Springer [Full text of this article is not available in the UHRA]
dc.description.abstractJets and winds in pre-main sequence (PMS) stars are often heated and ionized, and understanding their heating mechanism is desired to compare UV-to-IR spectral signatures with models and thus investigate their driving mechanism. We review our results of long-slit spectroscopy and spectro-astrometry for He I 1.083 μm and Hα emission, and investigate the heating mechanisms in the jet in the outer (>10 AU) and inner (<10 AU) regions, respectively.en
dc.relation.ispartofAstrophysics and Space Science
dc.subjectISM: jets and outflows
dc.titleHα and Hel emission in the jets of pre-main sequence stars : implications for the heating mechanismsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review

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