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dc.contributor.authorPustil'nik, S.A.
dc.contributor.authorLipovetsky, V.A.
dc.contributor.authorIzotov, Y.I.
dc.contributor.authorBrinks, E.
dc.contributor.authorThuan, T.X.
dc.contributor.authorKnyazev, A.Y.
dc.contributor.authorNeizvestnyi, S. I.
dc.contributor.authorUgryumov, A. V.
dc.date.accessioned2012-04-03T08:00:51Z
dc.date.available2012-04-03T08:00:51Z
dc.date.issued1997-05-01
dc.identifier.citationPustil'nik , S A , Lipovetsky , V A , Izotov , Y I , Brinks , E , Thuan , T X , Knyazev , A Y , Neizvestnyi , S I & Ugryumov , A V 1997 , ' Detection of a second optical component in the H I cloud of the young dwarf galaxy SBS 0335-052 : New observations with the 6-m telescope ' , Astronomy Letters , vol. 23 , pp. 308-311 .
dc.identifier.issn1562-6873
dc.identifier.otherPURE: 652342
dc.identifier.otherPURE UUID: d2bf3c10-52f8-4f6b-93d0-e0ef9dbd7406
dc.identifier.otherBibtex: urn:2a0d5744503a62662c659ff0a8cc3b94
dc.identifier.otherScopus: 0031478435
dc.identifier.otherORCID: /0000-0002-7758-9699/work/30407925
dc.identifier.urihttp://hdl.handle.net/2299/8150
dc.description.abstractThe Blue Compact Dwarf (BCD) galaxy SBS 0335–052 is one of the most metal–deficient galaxies known and one of the best candidates for a young dwarf galaxy in the process of formation. A VLA HI map reveals an unusual structure: the neutral gas is distributed in a very extended disk, about 15 times larger than the Holmberg optical diameter of the BCG. There are two peaks of high density. The eastern peak is close to the position of SBS 0335–052 whereas the western HI peak is associated with a faint compact optical galaxy. A 6–m telescope spectrum of this object shows H, H, and [OIII]5007 emission with a redshift close to that of SBS 0335–052. We suggest that it may be a young and chemically unevolved dwarf galaxy.en
dc.format.extent4
dc.language.isoeng
dc.relation.ispartofAstronomy Letters
dc.rightsOpen
dc.titleDetection of a second optical component in the H I cloud of the young dwarf galaxy SBS 0335-052 : New observations with the 6-m telescopeen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeSubmitted Version
dcterms.dateAccepted1997-05-01
rioxxterms.versionSMUR
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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