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dc.contributor.authorRiaz, Basmah
dc.contributor.authorThompson, M.A.
dc.contributor.authorWhelan, E.T.
dc.contributor.authorLodieu, N.
dc.date.accessioned2016-03-16T10:14:12Z
dc.date.available2016-03-16T10:14:12Z
dc.date.issued2015-01-21
dc.identifier.citationRiaz , B , Thompson , M A , Whelan , E T & Lodieu , N 2015 , ' Very low-luminosity Class I/flat outflow sources in sigma Orionis ' , Monthly Notices of the Royal Astronomical Society , vol. 446 , no. 3 , pp. 2550-2559 . https://doi.org/10.1093/mnras/stu2139
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 9618853
dc.identifier.otherPURE UUID: 253b0b2d-3dcc-445e-814c-9cd23c1976d6
dc.identifier.otherScopus: 84984950113
dc.identifier.otherORCID: /0000-0001-5392-909X/work/30970778
dc.identifier.urihttp://hdl.handle.net/2299/16782
dc.description.abstractWe present an optical to submillimetre multiwavelength study of two very low-luminosity Class I/flat systems, Mayrit 1701117 and Mayrit 1082188, in the σ Orionis cluster. We performed moderate-resolution (R ∼ 1000) optical (∼0.4–0.9 μm) spectroscopy with the Cassegrain Twin Spectrograph (TWIN) spectrograph at the Calar Alto 3.5-m telescope. The spectra for both sources show prominent emission in accretion- and outflow-associated linesen
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleVery low-luminosity Class I/flat outflow sources in sigma Orionisen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionScience & Technology Research Institute
dc.description.statusPeer reviewed
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnras/stu2139
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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