The Effect of the Bulge-to-disk Ratio on the Derived Opacities of Spiral Galaxies

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dc.contributor.authorTuffs, Richard J
dc.contributor.authorPopescu, Cristina C
dc.contributor.authorVolk, H J
dc.contributor.authorKylafis, Nikolaos
dc.contributor.authorDopita, Michael
dc.coverage.spatialPrague Czech Republic
dc.date.accessioned2015-12-13T23:09:09Z
dc.date.available2015-12-13T23:09:09Z
dc.date.createdSeptember 20 2004
dc.date.issued2004
dc.date.updated2015-12-12T08:17:48Z
dc.identifier.isbn0004-6337
dc.identifier.urihttp://hdl.handle.net/1885/86862
dc.publisherWiley-VCH Verlag GMBH
dc.relation.ispartofseriesAnnual Scientific Meeting of the Astronomische Gesellschaft and the Czech Astronomical Society
dc.sourceAsronomische Nachriten/Astronomical Notes vol. 325 Supp. Issue 1
dc.source.urihttp://www.lc.leidenuniv.nl/lc/web/2004/20040602/description.php3?wsid=97
dc.titleThe Effect of the Bulge-to-disk Ratio on the Derived Opacities of Spiral Galaxies
dc.typeConference paper
local.bibliographicCitation.lastpage119
local.bibliographicCitation.startpage118
local.contributor.affiliationTuffs, Richard J, Max Planck Institute for Nuclear Physics
local.contributor.affiliationPopescu, Cristina C, Max Planck Institute for Nuclear Physics
local.contributor.affiliationVolk, H J, Max Planck Institute for Nuclear Physics
local.contributor.affiliationKylafis, Nikolaos, University of Crete
local.contributor.affiliationDopita, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidDopita, Michael, u7501303
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub15903
local.type.statusPublished Version

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