Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-12-01T02:29:49.576Z Has data issue: false hasContentIssue false
  • English
  • Français

Review of abundances for mid-Teff range stars

Published online by Cambridge University Press:  25 May 2016

P.E. Nissen
P.E. Nissen*
Affiliation:
Institute of Physics and Astronomy University of Aarhus, DK-8000 Aarhus C, Denmark

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Among the mid-Teff (5000–7000 K) range stars, those on or near the main sequence are particularly important, because they provide much information on Galactic evolution and nucleosynthesis of the elements. This is due to the fact that these stars represent an age range from 0 to 15 Gyr, and a metallicity range from [Fe/H] ⋍ −4.0 to +0.3. Furthermore, it is likely that the present composition of elements in their atmospheres is similar to the composition of the interstellar gas from which they were formed, and that the present kinematics of the stars give information about their birthplaces. Hence, by observing selected samples of nearby F and G main sequence and subgiant stars one has the possibility to study the chemical and dynamical history of our Galaxy. Due to space limitation the present review is limited to these F and G stars. Supergiants are not discussed, but it should be emphasized, that their abundances are important for studies of advanced stellar evolutionary phases and determinations of the chemical composition of nearby galaxies. e.g. the Magellanic Clouds (Hill et al. 1995).

Type
Stellar Abundances
Information
Symposium - International Astronomical Union , Volume 189: Fundamental Stellar Properties: The Interaction Between Observation and Theory , 1997 , pp. 171 - 178
Copyright
Copyright © Kluwer 1997 

References

Anstee, S.D., O'Mara, B.J. 1995, MNRAS 276, 859 CrossRefGoogle Scholar
Anstee, S.D., O'Mara, B.J., Ross, J.E. 1997, MNRAS (in press) Google Scholar
Axer, M., Fuhrmann, K., Gehren, T. 1994, A&A 291, 895 Google Scholar
Bahcall, J.N., Pinsonneault, M.H. 1995, Rev. Mod. Phys. 67, 781 Google Scholar
Basu, S., Christensen-Dalsgaard, J., Schou, J., Thompson, M.J., Tomczyk, S. 1996, ApJ 460, 1064 Google Scholar
Bergbusch, P.A., VandenBerg, D.A. 1992, ApJS 81, 163 Google Scholar
Biémont, E., Baudoux, M., Kurucz, R.L., Ansbacher, W., Pinnington, E.H. 1991, A&A 249, 539 Google Scholar
Blackwell, D.E., Booth, A.J., Petford, A.D. 1984, A&A 132, 236 Google Scholar
Blackwell, D.E., Lynas-Gray, A.E., Smith, G. 1995, A&A 296, 217 Google Scholar
Boesgaard, A.M., Friel, E.D. 1990, ApJ 351, 467 Google Scholar
Cayrel, R., Cayrel de Strobel, G., Campbell, B. 1985, A&A 146, 249 Google Scholar
Dahn, C.C. 1994, in “Galactic and Solar System Optical Astrometry”, eds. Morrison, L.V. and Gilmore, G.F., Cambridge Univ. Press, p.55 Google Scholar
Edvardsson, B., Andersen, J., Gustafsson, B., Lambert, D.L., Nissen, P.E., Tomkin, J. 1993, A&A 275, 101 Google Scholar
Friel, E.D., Boesgaard, A.M. 1990, ApJ 351, 480 CrossRefGoogle Scholar
Garcia Lopez, R.J., Rebolo, R., Herrero, A., Beckman, J.E. 1993, ApJ 412, 173 Google Scholar
Hannaford, P., Lowe, R.M., Grevesse, N., Noels, A. 1992, A&A 259, 301 Google Scholar
Hill, V., Andrievsky, S., Spite, M. 1995, A&A 293, 347 Google Scholar
Holweger, H. 1996, Physica Scripta 65, 151 Google Scholar
Holweger, H., Müller, E.M. 1974, Solar Phys. 39, 19 CrossRefGoogle Scholar
Holweger, H., Heise, C., Kock, M. 1990, A&A 232, 510 Google Scholar
Holweger, H., Kock, M., Bard, A. 1995, A&A 296, 233 Google Scholar
King, J.R., Hiltgen, D.D. 1996, AJ 112, 2650 Google Scholar
Kiselman, D., Nordlund, Å. 1995, A&A 302, 578 Google Scholar
Kostik, R.I., Shchukina, N.G., Rutten, R.J. 1996, A&A 305, 325 Google Scholar
Kurucz, R.L. 1993, CD-ROM 13, Smithsonian Astrophys. Obs. Google Scholar
Kurucz, R.L. 1995, ApJ 452, 102 Google Scholar
Lambert, D.L. 1978, MNRAS 182, 249 Google Scholar
Magain, P. 1989, A&A 209, 211 Google Scholar
Milford, P.N., O'Mara, B.J., Ross, J.E. 1994, A&A 292, 276 Google Scholar
Nissen, P.E., Schuster, W.J. 1997, A&A (submitted) Google Scholar
Nissen, P.E., Gustafsson, B., Edvardsson, B., Gilmore, G. 1994, A&A 285, 440 Google Scholar
Norris, J.E., Ryan, S.G., Stringfellow, G.S. 1994, ApJ 423, 386 Google Scholar
Pilachowski, C.A., Sneden, C., Booth, J. 1993, ApJ 407, 699 Google Scholar
Proffitt, C.R. 1994, ApJ 425, 849 CrossRefGoogle Scholar
Ryan, S.G., Norris, J.E., Beers, T.C. 1996, ApJ 471, 254 Google Scholar
Tomkin, J., Lemke, M., Lambert, D.L., Sneden, C. 1992, AJ 104, 1568 Google Scholar
Thorburn, J.A. 1994, ApJ 421, 318 Google Scholar
Sauval, A.J., Grevesse, N., Brault, J.W., Stokes, G.M., Zander, R. 1984, ApJ 282, 330 Google Scholar
Schuster, W.J., Parrao, L., Contreras Martinez, M.E. 1993, A&AS 97, 951 Google Scholar
Songaila, A., Cowie, L.L., Hogan, C.J., Rugers, M. 1994, Nature 368, 599 Google Scholar
Spite, M., François, P., Nissen, P.E., Spite, F. 1996, A&A 307, 172 Google Scholar