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Current assessment of the Red Rectangle band problem

dc.contributor.authorGlinski, R J
dc.contributor.authorMichaels, P
dc.contributor.authorAnderson, C M
dc.contributor.authorSchmidt, Timothy W.
dc.contributor.authorSharp, Robert
dc.contributor.authorSitko, Michael L
dc.contributor.authorBernstein, L S
dc.contributor.authorvan Winckel, Hans
dc.date.accessioned2015-12-13T22:48:42Z
dc.date.issued2009
dc.date.updated2016-02-24T09:42:27Z
dc.description.abstractIn this paper we discuss our insights into several key problems in the identification of the Red Rectangle Bands (RRBs). We have combined three independent sets of observations in order to try to define the constraints guiding the bands. We provide a summary of the general behavior of the bands and review the evidence for a molecular origin of the bands. The extent, composition, and possible absorption effects of the bands are discussed. Comparison spectra of the strongest band obtained at three different spectral resolutions suggests that an intrinsic line width of individual rotational lines can be deduced. Spectroscopic models of several relatively simple molecules were examined in order to investigate where the current data are weak. Suggestions are made for future studies to enhance our understanding of these enigmatic bands.
dc.identifier.issn0004-640X
dc.identifier.urihttp://hdl.handle.net/1885/80204
dc.publisherKluwer Academic Publishers
dc.sourceAstrophysics and Space Science
dc.subjectKeywords: Astrochemistry; Circumstellar matter; Line: Identification; Line: Profiles; Stars: late-type
dc.titleCurrent assessment of the Red Rectangle band problem
dc.typeJournal article
local.bibliographicCitation.issue4
local.bibliographicCitation.lastpage344
local.bibliographicCitation.startpage337
local.contributor.affiliationGlinski, R J, Tennessee Tech University
local.contributor.affiliationMichaels, P, Tennessee Tech University
local.contributor.affiliationAnderson, C M, University of Wisconsin
local.contributor.affiliationSchmidt, Timothy W., University of Sydney
local.contributor.affiliationSharp, Robert, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSitko, Michael L, University of Cincinnati
local.contributor.affiliationBernstein, L S, Spectral Sciences, Inc
local.contributor.affiliationvan Winckel, Hans, Instituut voor Sterrenkunde
local.contributor.authoruidSharp, Robert, u4954956
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf5625xPUB8500
local.identifier.citationvolume323
local.identifier.doi10.1007/s10509-009-0084-9
local.identifier.scopusID2-s2.0-70350211849
local.type.statusPublished Version

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