dc.creator |
Guenther, David B. |
|
dc.creator |
Demarque, P. |
|
dc.date.accessioned |
2015-02-03T18:14:53Z |
|
dc.date.available |
2015-02-03T18:14:53Z |
|
dc.date.issued |
1996-01 |
|
dc.identifier.issn |
0004-637X |
|
dc.identifier.uri |
http://library2.smu.ca/xmlui/handle/01/25939 |
|
dc.description |
Publisher's version/PDF |
en_CA |
dc.description.abstract |
The p-mode frequencies recently observed by Kjeldsen and coworkers, along with other observables, are used to determine the mass, age, and helium abundance of [eta] Bootis. We show, by direct application, how the p-model frequencies and stellar seismological tools aid in constraining the physical parameters of [eta] Boo. We confirm the existence of mode bumping and discuss how it may be used to refine the estimate of [eta] Boo's age. We describe the effect of the new OPAL equation-of-state tables (Rogers, Swenson, and Iglesias) on the p-mode frequencies. |
en_CA |
dc.description.provenance |
Submitted by Janine Mills (janine.mills@smu.ca) on 2015-02-03T18:14:53Z
No. of bitstreams: 1
Guenther_David_B_article_1996.pdf: 276513 bytes, checksum: ab21ddbd5a9066f46052d0be5bc89e4d (MD5) |
en |
dc.description.provenance |
Made available in DSpace on 2015-02-03T18:14:53Z (GMT). No. of bitstreams: 1
Guenther_David_B_article_1996.pdf: 276513 bytes, checksum: ab21ddbd5a9066f46052d0be5bc89e4d (MD5)
Previous issue date: 1996-01 |
en |
dc.language.iso |
en |
en_CA |
dc.publisher |
American Astronomical Society |
en_CA |
dc.relation.uri |
http://dx.doi.org/10.1086/176698 |
|
dc.rights |
Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user. |
|
dc.subject.lcsh |
Stars -- Evolution |
|
dc.subject.lcsh |
Subgiant stars |
|
dc.subject.lcsh |
Stars -- Structure |
|
dc.subject.lcsh |
Stellar oscillations |
|
dc.title |
Seismology of [eta] Bootis |
en_CA |
dc.type |
Text |
en_CA |
dcterms.bibliographicCitation |
Astrophysical Journal 456, 798-810. (1996) |
en_CA |
Copyright statement:
Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user.