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dc.contributor.authorRodrigues, I.
dc.contributor.authorDottori, H.
dc.contributor.authorBrinks, E.
dc.contributor.authorMirabel, F.
dc.date.accessioned2007-10-23T14:21:53Z
dc.date.available2007-10-23T14:21:53Z
dc.date.issued1999
dc.identifier.citationRodrigues , I , Dottori , H , Brinks , E & Mirabel , F 1999 , ' Study of the interacting system NGC 6845 ' , The Astronomical Journal , vol. 117 , no. 6 , pp. 2695-2708 .
dc.identifier.issn0004-6256
dc.identifier.otherPURE: 168567
dc.identifier.otherPURE UUID: 7e8f7c4e-9946-4663-8061-8ade74bc1dd6
dc.identifier.otherdspace: 2299/972
dc.identifier.otherScopus: 0038875932
dc.identifier.otherORCID: /0000-0002-7758-9699/work/30407912
dc.identifier.urihttp://hdl.handle.net/2299/972
dc.descriptionOriginal article can be found at: http://www.journals.uchicago.edu/AJ/--Copyright American Astronomical Society
dc.description.abstractWe present optical spectroscopy, B, V , R, and I CCD photometry, and VLA neutral hydrogen observations of the interacting quartet NGC 6845, also know as Klemola 30. NGC 6845 A, the dominant component, sports a broad and bright tidal bridge and a faint tidal tail, which bifurcates. The tidal bridge has a B[I color bluer than that of the inner disk of NGC 6845 A. Five strong condensations, identified as H II regions brighter than the brightest one known in our Galaxy, are found along the tidal bridge, with the two most luminous located at the bridge tip. Two giant H II regions, comparable to 30 Dor, are located where the tidal bridge and the tidal tail join the disk of NGC 6845 A.en
dc.language.isoeng
dc.relation.ispartofThe Astronomical Journal
dc.rightsOpen
dc.titleStudy of the interacting system NGC 6845en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1999
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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