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The Formation and Evolution of White Dwarfs

Published online by Cambridge University Press:  25 April 2016

M. S. Bessell
M. S. Bessell*
Affiliation:
Mount Stromlo and Siding Spring Observatories Australian National University
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Extract

A white dwarf is a body of stellar mass, but of planetary dimensions. It is self luminous with a surface temperature that has been observed as high as 70,000 K or as low as 4,000 K. Because of its low surface area the star is far fainter than a main sequence star of the same colour; equally the light it emits is bluer than that from a main sequence star of similar luminosity. Figure 1 is the HR diagram from data obtained by the US Naval Observatory showing the dwarf and white dwarf sequences.

Type
Invited Papers
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 3 , 1978 , pp. 220 - 224
Copyright
Copyright © Astronomical Society of Australia 1978

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References

Bessell, M. S., and Wickramasinghe, D. T., Mon. Noi. Roy. Astron. Soc, 182, 275 (1978).Google Scholar
Bessell, M. S., and Wickramasinghe, D. T., Pub. Astron. Soc. Pac. (submitted on the existence of DA, F stars) (1978).Google Scholar
Chandrasekhar, S., Stellar Structure (Chicago: University of Chicago Press) (1939).Google Scholar
Cottrell, P. L., Bessell, M. S., and Wickramasinghe, D. T., Astrophys. J. (Letters), 218, L133 (1977).CrossRefGoogle Scholar
Eddington, A. S., The Internal Constitution of Stars (Cambridge: University Press) (1926).Google Scholar
Fowler, R. H., Mon. Not. Roy. Astron. Soc, 87, 114 (1926).Google Scholar
Greenstein, J. L., Astron. J., 81, 323 (1976).Google Scholar
Harm, R., and Schwarzchild, M., Astrophys. J., 200, 324 (1975).Google Scholar
Iben, I., Annu. Rev. Astron. & Astrophys., 12, 215 (1974).Google Scholar
Keeley, D. A., Astrophys. J., 161, 643 (1970).CrossRefGoogle Scholar
Koester, D., Astron. & Astrophys., 12, 2125 (1974).Google Scholar
McCook, G. P., and Sion, E. M., Villanova University Contributions No. 2 (1977).Google Scholar
Mewe, R., Heise, J., Gronenschild, E. J. B. M., Brinkman, A. C., Schryver, J., den Boggende, A. J. F., Astrophys. J. (Letters), 202, L67 (1975).CrossRefGoogle Scholar
O’Dell, C. R., IAU Symposium No. 34 (ed. Osterbrock, D. E. and O’Dell, C. R.: Dordrecht-Holland: D. Reidel Publishing Company) p. 361 (1968).Google Scholar
Paczynski, B., Acta. Astron., 21, 417 (1971).Google Scholar
Pottasch, S. R., Wu, C. C, Wesselius, P. R., Fieten, H., Van Huiten, R. J., Astron & Astrophys. (in press 1978).Google Scholar
Reimers, D., in 19th Liege International Astrophysical Colloquium, p. 369 (1975).Google Scholar
Shaviv, G., and Kovetz, A., Astron. & Astrophys., 51, 383 (1976).Google Scholar
Sion, E. M., and Liebert, J., Astrophys. J., 213, 468 (1977).Google Scholar
Sweeney, M. A., Astron. & Astrophys., 49, 375 (1976).Google Scholar
Vauclair, G., and Reisse, C., Astron. & Astrophys., 61, 415 (1977).Google Scholar
Weidemann, V., Astron. & Astrophys., 61, L27 (1977).Google Scholar
Wickramasinghe, D. T., Bessell, M. S., and Cottrell, P. L., Astrophys. J. (Letters), 217, L65 (WBC I 1977).Google Scholar
Wickramasinghe, D. T., Bessell, M. S., and Cottrell, P. L., “Cool White Dwarfs and the Red Deficit Problem” (WBC II) (In preparation for Astrophys. J., 1979).Google Scholar
Wickramasinghe, D. T., & Bessell, M. S., Mon. Not. Roy. Astron. Soc, 181, 713 (1977).Google Scholar
Wood, P. R., Astrophys. J., 190, 609 (1974).Google Scholar
Wood, P. R., and Cahn, J. H., Astrophys. J., 211, 499 (1977).Google Scholar