Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-23T15:50:02.087Z Has data issue: false hasContentIssue false

Observations Bearing on the Theory of Stellar Convection II

Published online by Cambridge University Press:  15 February 2018

Erika Böhm-Vitense*
Affiliation:
University of Washington, Seattle, Wa., U.S.A., and University of Göttingen, Germany

Summary

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.

It is shown that the best way to get information about efficiency of convective energy transport in the hydrogen convection zones in stars other than the sun is presently contained in continuous energy distributions of A and F stars. Scans show that convective energy transport must be much more efficient than thought hitherto. The scans indicate that rapid rotation enhances convective energy transport.

Figure 1 lists all the observations, we could think of, which are influenced by the outer convection zone and which can therefore give us information for our convection theory.

Type
I. Mixing-Length Theory
Copyright
Copyright © 1976

References

Abt, H. and Hunter, J.: 1962, Ap. J. 13638, 381 CrossRefGoogle Scholar
Allen, L.H., Greenstein, J.L.: 1960, Ap. J. Suppl. 538, 139 Google Scholar
Andersen, P.: 1973, P.A.S.P. 8538, 666 Google Scholar
Andersen, C.M., Stoeckley, R. and Kraft, R.P.: 1966, Ap. J. 14338, 299 CrossRefGoogle Scholar
Baschek, B. and Oke, J.B.: 1965, Ap. J. 14138, 1404 CrossRefGoogle Scholar
Baschek, B. and Reimers, D.: 1969, Astron. and Astrophys. 238, 240 Google Scholar
Böhm, K.H.: 1958, Zs. f. Ap. 4638, 245 Google Scholar
Böhm-Vitense, E.: 1970a, Astron. and Astrophys. 838, 283 Google Scholar
Böhm-Vitense, E.: 1970b, Astron. and Astrophys. 838, 209 Google Scholar
Böhm-Vitense, E. and Szkody, P.: 1974, Ap. J. 19338, 607 Google Scholar
Böhm-Vitense, E. and Canterna, R.: 1975, Ap. J. 19438, 629 Google Scholar
Böhm-Vitense, E. and Nelson, G.: 1976, Ap. J. in pressGoogle Scholar
Böhm-Vitense, E. and Johnson, P.: 1977, in preparationGoogle Scholar
Canterna, R.: 1976, private communicationGoogle Scholar
Chaffee, R.H.: 1970, Astron. and Astrophys. 438, 291 Google Scholar
Chandrasekhar, S. : 1961, Hydrodynamic and Hydromagnetic Stability (Oxford, Clarendon Press) p. 135 Google Scholar
Collins, G.W.: 1965, Ap. J. 14238, 265 Google Scholar
Dickens, R. J., Kraft, R. P., and Krzeminski, W. : 1968, A . J. 7338, 6 Google Scholar
Frisch, H. and U., : 1975, Physique des Mouvements dans les Atmosphères Stellaires (Centre National de la Recherche Scientifique, Paris 1976)Google Scholar
Garz, T. and Kock, M.: 1969, Astron. and Astrophys. 238, 274 Google Scholar
Hayes, D.S. and Lantham, D.W.: 1975, Ap. J. 19738, 593 Google Scholar
Hoyle, F. and Schwarzschild, M.: 1955, Ap. J. Suppl. 1338 Google Scholar
Huang, S. and Struve, O.: 1952, Ap. J. 11638, 410 Google Scholar
Iben, I.: 1963, Ap. J. 13838, 452 Google Scholar
Johnson, H.L.: 1952, Ap. J. 11638, 640 Google Scholar
Johnson, H.L. and Morgan, W. W.: 1953, Ap. J. 11738, 313 Google Scholar
Johnson, H.L. and Knuckles, C.F.: 1955, Ap. J. 12238, 209 Google Scholar
Johnson, H.L. and Mitchell, R.I.: 1958, Ap. J. 12838, 31 Google Scholar
Johnson, H.L., Mitchell, R.I. and Iriarte, B.: 1962, Ap. J. 13638, 75 Google Scholar
Johnson, H.L., Mitchell, R.I., Iriarte, B., and Wisniewski, W.: 1966, Comm. Lunar and Planet. Lab. No. 63 Google Scholar
Kippenhahn, R.: 1972, In Stellar Chromospheres, Proceedings of NASA Colloquium.Google Scholar
Slettebak, A.: 1955, Ap. J. 12138, 653 Google Scholar
Strömgren, B. and Perry, C. : 1965, unpublished report. Institute of Advanced Study, Princeton, N.J.Google Scholar
Traving, G.: 1975, Physique des Mouvements dans les Atmospheres Stellaires (Centre National de la Recherche Scientifique, Paris 1976)Google Scholar
Wallerstein, G.: 1962, Ap. J. Suppl. 638, 407 Google Scholar
Wallerstein, G. and Heifer, H.L.: 1966 Ap. J. 7138, 350 Google Scholar
Wilson, O.C.: 1976, Ap. J. 20538, 823 Google Scholar
Wright, K.O.: 1955, Transactions of the IAU, IX38, 739 Google Scholar
Zirin, H.: 1975, Reprint, Hale Observatories (Carnegie Institution of Washington, California Institute of Technology, BBSO No. 0150)Google Scholar
Kraft, R.P.: 1965, Ap. J. 14238, 681 Google Scholar
Kraft, R.P.: 1967, Ap. J. 14838, 129 Google Scholar
Lucy, L.B.: 1976, Ap. J. 20638, 499 Google Scholar
Mannery, E.J., Wallerstein, G. and Welch, G.A.: 1968, Ap. J. 7338, 548 Google Scholar
Matsushima, S. and Travis, L.D.: 1973, Ap. J. 18138, 387 Google Scholar
Mendoza, E.E.: 1956, Ap. J. 12338, 54 Google Scholar
Mitchell, R.I.: 1960, Ap. J. 13238, 68 Google Scholar
Oke, J.B.: 1964, Ap. J. 14038, 689 Google Scholar
Oke, J.B. and Conti, P. S.: 1966, Ap. J. 14338, 134 Google Scholar
Oke, J.B. and Schild, R. E.: 1970, Ap. J. 16138, 1015 Google Scholar
Paradijs, J. van: 1973, Astron. and Astrophys. 2338, 369 Google Scholar
Reimers, D.: 1976, Physique des Mouvements dans les Atmospheres Stellaires. (Centre National de la Recherche Scientifique, Paris 1976)Google Scholar
Rosendhal, J.: 1910, Ap. J. 16038, 627 Google Scholar
Sandage, A. and Tammann, G.A.: 1971, Ap. J. 16738, 293 Google Scholar
Schwarzschild, M.: 1975, Ap. J. 19538, 137 Google Scholar
Sedlmayr, E.: 1975, Physique des Mouvements dans les Atmosphlres Stellaires. (Centre National de la Recherche Scientifique, Paris 1976)Google Scholar