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dc.contributor.authorMolina, C. Navarro
dc.contributor.authorBorissova, J.
dc.contributor.authorCatelan, M.
dc.contributor.authorLucas, P. W.
dc.contributor.authorMedina, N.
dc.contributor.authorPena, C. Contreras
dc.contributor.authorKurtev, R.
dc.contributor.authorMinniti, D.
dc.date.accessioned2020-03-25T01:09:00Z
dc.date.available2020-03-25T01:09:00Z
dc.date.issued2019-02
dc.identifier.citationMolina , C N , Borissova , J , Catelan , M , Lucas , P W , Medina , N , Pena , C C , Kurtev , R & Minniti , D 2019 , ' Long-term Stellar Variability in the Galactic Centre Region ' , Monthly Notices of the Royal Astronomical Society , vol. 482 , no. 4 , sty3041 , pp. 5567–5586 . https://doi.org/10.1093/mnras/sty3041
dc.identifier.issn0035-8711
dc.identifier.otherArXiv: http://arxiv.org/abs/1811.01897v1
dc.identifier.otherORCID: /0000-0002-8872-4462/work/71186143
dc.identifier.urihttp://hdl.handle.net/2299/22474
dc.description© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society.
dc.description.abstractWe report the detection of variable stars within a 11.5' x 11.5' region near the Galactic centre (GC) that includes the Arches and Quintuplet clusters, as revealed by the VISTA Variables in the Via Lactea (VVV) survey. There are 353 sources that show Ks-band variability, of which the large majority (81%) correspond to red giant stars, mostly in the asymptotic giant branch (AGB) phase. We analyze a population of 52 red giants with long-term trends that cannot be classified into the typical pulsating star categories. Distances and extinctions are calculated for 9 Mira variables, and we discuss the impact of the chosen extinction law on the derived distances. We also report the presence of 48 new identified young stellar object (YSO) candidates in the region.en
dc.format.extent22
dc.format.extent7146596
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectastro-ph.SR
dc.titleLong-term Stellar Variability in the Galactic Centre Regionen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1093/mnras/sty3041
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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