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dc.contributor.authorGkouvelis, L.
dc.contributor.authorFabregat, J.
dc.contributor.authorZorec, J.
dc.contributor.authorSteeghs, D.
dc.contributor.authorDrew, J. E.
dc.contributor.authorRaddi, R.
dc.contributor.authorWright, N. J.
dc.contributor.authorDrake, J. J.
dc.date.accessioned2018-06-08T15:29:51Z
dc.date.available2018-06-08T15:29:51Z
dc.date.issued2016-07-01
dc.identifier.citationGkouvelis , L , Fabregat , J , Zorec , J , Steeghs , D , Drew , J E , Raddi , R , Wright , N J & Drake , J J 2016 , ' Physical parameters of IPHAS-selected classical Be stars. (I. Determination procedure and evaluation of the results.) ' , Astronomy & Astrophysics , vol. 591 , A140 . https://doi.org/10.1051/0004-6361/201527090
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 10311283
dc.identifier.otherPURE UUID: ac6eba67-16c9-45d8-961d-afad20ba288f
dc.identifier.otherArXiv: http://arxiv.org/abs/1604.05935v1
dc.identifier.otherScopus: 84977489417
dc.identifier.urihttp://hdl.handle.net/2299/20173
dc.descriptionReproduced with permission from Astronomy & Astrophysics, © 2016 ESO
dc.description.abstractWe present a semi-automatic procedure to obtain fundamental physical parameters and distances of classical Be (CBe) stars, based on the Barbier-Chalonge-Divan (BCD) spectrophotometric system. Our aim is to apply this procedure to a large sample of CBe stars detected by the IPHAS photometric survey, to determine their fundamental physical parameters and to explore their suitability as galactic structure tracers. In this paper we describe the methodology used and the validation of the procedure by comparing our results with those obtained from different independent astrophysical techniques for subsamples of stars in common with other studies. We also present a test case study of the galactic structure in the direction of the Perseus Galactic Arm, in order to compare our results with others recently obtained with different techniques and the same sample of stars. We did not find any significant clustering of stars at the expected positions of the Perseus and Outer Galactic Arms, in agreement with previous studies in the same area that we used for verification.en
dc.format.extent18
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysics
dc.rightsOpen
dc.subjectastro-ph.SR
dc.subjectPhysics and Astronomy(all)
dc.titlePhysical parameters of IPHAS-selected classical Be stars. (I. Determination procedure and evaluation of the results.)en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.description.versiontypeFinal Published version
dcterms.dateAccepted2016-07-01
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1051/0004-6361/201527090
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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