An examination of the planetesimal impact hypothesis of the formation of CP stars
dc.contributor.author | Cowley, Charles R. | en_US |
dc.date.accessioned | 2006-09-08T19:58:44Z | |
dc.date.available | 2006-09-08T19:58:44Z | |
dc.date.issued | 1977-10 | en_US |
dc.identifier.citation | Cowley, 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.issn | 0004-640X | en_US |
dc.identifier.issn | 1572-946X | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/42108 | |
dc.description.abstract | The 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.extent | 896153 bytes | |
dc.format.extent | 3115 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.language.iso | en_US | |
dc.publisher | Kluwer Academic Publishers; D. Reidel Publishing Company ; Springer Science+Business Media | en_US |
dc.subject.other | Physics | en_US |
dc.subject.other | Astronomy | en_US |
dc.title | An examination of the planetesimal impact hypothesis of the formation of CP stars | en_US |
dc.type | Article | en_US |
dc.subject.hlbsecondlevel | Astronomy | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | University of Victoria and Dominion Astrophysical Observatory, Victoria, B.C., Canada; University of Michigan, Ann Arbor, Mich., USA | en_US |
dc.contributor.affiliationumcampus | Ann Arbor | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/42108/1/10509_2004_Article_BF00644158.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1007/BF00644158 | en_US |
dc.identifier.source | Astrophysics and Space Science | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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