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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.otherdspace: 2299/972
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.format.extent2010348
dc.language.isoeng
dc.relation.ispartofThe Astronomical Journal
dc.titleStudy of the interacting system NGC 6845en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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