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An examination of the planetesimal impact hypothesis of the formation of CP stars

dc.contributor.authorCowley, Charles R.en_US
dc.date.accessioned2006-09-08T19:58:44Z
dc.date.available2006-09-08T19:58:44Z
dc.date.issued1977-10en_US
dc.identifier.citationCowley, Charles R.; (1977). "An examination of the planetesimal impact hypothesis of the formation of CP stars." Astrophysics and Space Science 51(2): 349-362. <http://hdl.handle.net/2027.42/42108>en_US
dc.identifier.issn0004-640Xen_US
dc.identifier.issn1572-946Xen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/42108
dc.description.abstractThe impact hypothesis has been found to provide a qualitative basis for an understanding of many of the characteristics of the CP stars. It founders primarily upon the problem of underabundances of certain elements and large variations in isotopic abundances. We conclude, however, that the hypothesis should not be prematurely discarded, since it may be combined with other mechanisms to account for the variety of abundance peculiarities of the CP stars.en_US
dc.format.extent896153 bytes
dc.format.extent3115 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherKluwer Academic Publishers; D. Reidel Publishing Company ; Springer Science+Business Mediaen_US
dc.subject.otherPhysicsen_US
dc.subject.otherAstronomyen_US
dc.titleAn examination of the planetesimal impact hypothesis of the formation of CP starsen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumUniversity of Victoria and Dominion Astrophysical Observatory, Victoria, B.C., Canada; University of Michigan, Ann Arbor, Mich., USAen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/42108/1/10509_2004_Article_BF00644158.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF00644158en_US
dc.identifier.sourceAstrophysics and Space Scienceen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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