dc.contributor.author | Riaz, Basmah | |
dc.contributor.author | Thompson, M.A. | |
dc.contributor.author | Whelan, E.T. | |
dc.contributor.author | Lodieu, N. | |
dc.date.accessioned | 2016-03-16T10:14:12Z | |
dc.date.available | 2016-03-16T10:14:12Z | |
dc.date.issued | 2015-01-21 | |
dc.identifier.citation | Riaz , 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.issn | 0035-8711 | |
dc.identifier.other | PURE: 9618853 | |
dc.identifier.other | PURE UUID: 253b0b2d-3dcc-445e-814c-9cd23c1976d6 | |
dc.identifier.other | Scopus: 84984950113 | |
dc.identifier.other | ORCID: /0000-0001-5392-909X/work/30970778 | |
dc.identifier.uri | http://hdl.handle.net/2299/16782 | |
dc.description.abstract | We 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 lines | en |
dc.language.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
dc.title | Very low-luminosity Class I/flat outflow sources in sigma Orionis | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.contributor.institution | Centre for Astrophysics Research | |
dc.contributor.institution | Science & Technology Research Institute | |
dc.description.status | Peer reviewed | |
rioxxterms.version | AM | |
rioxxterms.versionofrecord | https://doi.org/10.1093/mnras/stu2139 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |