Skip to main content Accessibility help
×
Home

Elemental Abundances of Sharp-Lined Metallic-Lined and Comparable Normal Stars

  • Dursun Koçer (a1), Saul J. Adelman (a2), Çetin Bolcal (a3) and Graham Hill (a4)

Abstract

We are performing elemental abundances of sharp-lined metallic-lined stars and normal late A through middle F stars using 2.4 Å mm−1 photographic region spectrograms taken with the coudé spectrograph of the 1.4-m telescope of the Dominion Astrophysical Observatory. Our initial studies of the Am stars 15 Vul and 32 Aqr and the normal stars θ Cyg (F4 V) and ɩ Psc (F7 V) showed that the elemental abundances of the normal stars were close to solar while 15 Vul shows smaller abundance anomalies than does 32 Aqr. These analyses are being done consistently with SJA’s studies of the HgMn and hotter normal stars.

    • Send article to Kindle

      To send this article to your Kindle, first ensure no-reply@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about sending to your Kindle. Find out more about sending to your Kindle.

      Note you can select to send to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be sent to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

      Find out more about the Kindle Personal Document Service.

      Elemental Abundances of Sharp-Lined Metallic-Lined and Comparable Normal Stars
      Available formats
      ×

      Send article to Dropbox

      To send this article to your Dropbox account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Dropbox.

      Elemental Abundances of Sharp-Lined Metallic-Lined and Comparable Normal Stars
      Available formats
      ×

      Send article to Google Drive

      To send this article to your Google Drive account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Google Drive.

      Elemental Abundances of Sharp-Lined Metallic-Lined and Comparable Normal Stars
      Available formats
      ×

Copyright

Corresponding author

* Guest Investigator, Dominion Astrophysical Observatory, Hertzberg Institute of Astrophysics, National Research Council of Canada

References

Hide All
Adelman, S.J. 1991, MNRAS, 252, 116
Adelman, S.J., Bolcal, C., Hill, G., and Koçer, D. 1991. MNRAS, 252, 329
Adelman, S.J., and Hill, G. 1987, MNRAS, 226, 581
Anders, E., and Grevesse, N. 1989, Geochim. Cosmochim. Acta, 53, 197
Bolcal, C., Koçer, D., and Adelman, S.J. 1992, MNRAS, in press
Cowley, C.R., and Adelman, S.J. 1990, PASP, 102, 1077
Fuhr, J.R., Martin, G.A., and Wiese, W.L. 1988, J. Phys. Chem. Ref. Data, 17, Suppl. 4
Hill, G., and Fisher, W.A. 1986, Publ. Dom. Astrophys. Obs., 16, 159
Lane, M.C., and Lester, J.B. 1987, ApJS, 65, 137
Kurucz, R.L. 1979, ApJS, 40, 1
Moon, T.T., and Dworetsky, M.M. 1985, MNRAS, 217, 305

Elemental Abundances of Sharp-Lined Metallic-Lined and Comparable Normal Stars

  • Dursun Koçer (a1), Saul J. Adelman (a2), Çetin Bolcal (a3) and Graham Hill (a4)

Metrics

Full text views

Total number of HTML views: 0
Total number of PDF views: 0 *
Loading metrics...

Abstract views

Total abstract views: 0 *
Loading metrics...

* Views captured on Cambridge Core between <date>. This data will be updated every 24 hours.

Usage data cannot currently be displayed