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The Baade-Wesselink Technique

Published online by Cambridge University Press:  12 April 2016

Thomas J. Moffett*
Affiliation:
Department of Physics, Purdue University, West Lafayette, Indiana, 47907

Extract

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The historical foundations of the Baade-Wesselink (BW) method were established through the work of Baade (1926), Becker (1940), and Wesselink (1947). All modern versions of the BW-method are constructed upon these foundations. Since the radii of pulsating stars are fundamental to many areas of astronomical research (theories of stellar structure and evolution, galactic structure, and the cosmic distance scale), it is paramount that we strive to improve their observational determination. At the present time, the BW-technique is the only “direct” method for determining the radii of pulsating stars. Until a new technique is devised, better determinations of this important physical parameter will only occur through improvements in the BW-method.

Type
3. Comparison of the Milky Way with Other Galaxies
Copyright
Copyright © Cambridge University Press 1989

References

Baade, W. (1926). Astron. Nachr., 228, 359.Google Scholar
Balona, L.A. (1977). M.N.R.A.S., 178, 231.CrossRefGoogle Scholar
Balona, L.A. & Martin, W.L. (1978a). M.N.R.A.S., 184, 1.Google Scholar
Balona, L.A. & Martin, W.L. (1978b). M.N.R.A.S., 184, 11.CrossRefGoogle Scholar
Barnes, T.G., Dominy, J.F.,Evans, D.S., Kelton, P.W., Parsons, S.B. & Stover, R.J. (1977). M.N.R.A.S., 178, 661.CrossRefGoogle Scholar
Barnes, T.G., Evans, D.S. & Moffett, T.J. (1978). M.N.R.A.S., 183, 285.Google Scholar
Barnes, T.G., Moffett, T.J., Jefferys, W.H. & Hawley, S.L. (1987). Bull.Amer. Astron. Soc., 19, 754.Google Scholar
Becker, W. (1940). Zeitschr. f. Astrophys, 19, 269.Google Scholar
Bell, R.A. & Gustafsson, B. (1980). M.N.R.A.S., 191, 435.CrossRefGoogle Scholar
Burki, G. & Benz, W. (1982). Astron. & Astrophys., 115, 30.Google Scholar
Burki, G. & Meylan, G. (1986). Astron. Astrophys., 156, 131.Google Scholar
Caccin, B., Onnembo, A., Russo, G. & Sollazzo, C. (1981). Astron. Astrophys., 97, 104.Google Scholar
Carney, B.W. & Latham, D.W. (1984). Ap. J., 278, 241.CrossRefGoogle Scholar
Cohen, J.G. & Gordon, G.A. (1987). Ap. J., 318, 215.CrossRefGoogle Scholar
Coulson, I.M., Caldwell, J.A.R. & Gieren, W.P. (1986). Ap.J., 303, 273.Google Scholar
Fernley, J.A., Longmore, A.J. & Jameson, R.F. (1987). In Stellar Pulsation: A Memorial to John Cox, P., eds. Cox, A.N., Sparks, W.M., and Starrfield, S.G.. p. 239. Berlin: Springer-Verlag.Google Scholar
Fernley, J.A., Lynas-Gray, A.E., Skillen, I., Jameson, R.F., Marang, F., Kilkenny, D. & Longmore, A.J. (1988). M.N.R.A.S., (in press).Google Scholar
Gautschy, A. (1987). Vistas in Astronomy, 30, 197.Google Scholar
Gieren, W. P. (1986). M.N.R.A.S., 222, 251.CrossRefGoogle Scholar
Hawley, S.L., Barnes, T.G. & Moffett, T.J. (1987). In Stellar Pulsation: A Memorial to Cox, John P., eds. Cox, A.N., Sparks, W.M., and Starrfield, S.G., p. 235. Berlin: Springer-Verlag.Google Scholar
Hindsley, R. & Bell, R.A. (1987). In Stellar Pulsation: A Memorial to Cox, John P., eds. Cox, A.N., Sparks, W.M., and Starrfield, S.G., p. 212. Berlin: Springer-Verlag.Google Scholar
Jones, R.V. (1988). Ap. J., 326, 305.Google Scholar
Jones, R.V., Carney, B.W. & Latham, D.W. (1988). Ap. J., 326, 312.Google Scholar
Jones, R.V., Carney, B.W., Latham, D.W. & Kurucz, R.L. (1987a). Ap.J., 312, 254.CrossRefGoogle Scholar
Jones, R.V., Carney, B.W., Latham, D.W. & Kurucz, R.L. (1987b). Ap.J., 314, 605.Google Scholar
Kurucz, R.L. (1979). Ap. J. Suppl., 40, 1.Google Scholar
Liu, T. & Janes, K.A. (1988). In Calibrating Stellar Ages, Contributions of the Van Vleck Observatory No. 6, ed. Philips, A.G.D., (in press). Schenectady, N.Y.: L. Davis Press.Google Scholar
Manduca, A., Bell, R.A., Barnes, T.G., Moffett, T.J. & Evans, D.S. (1981). Ap. J., 250, 312.Google Scholar
McNamara, D.H. & Feltz, K.A. (1977). P.A.S.P., 89, 699.Google Scholar
Moffett, T.J. & Barnes, T.G. (1987). Ap.J., 323, 280.Google Scholar
Onnembo, A., Buonaura, B., Caccin, B., Russo, G. & Sollazzo, C. (1985). Astron. & Astrophys., 152, 349.Google Scholar
Simon, N.R. (1987). P.A.S.P., 99, 868.Google Scholar
Simon, N.R. (1988). M.N.R.A.S., (in press).Google Scholar
Sollazzo, C., Russo, G., Onnembo, A. & Caccin, B. (1981). Astron. & Astrophys., 99, 66.Google Scholar
Thompson, R.J. (1975). M.N.R.A.S., 172, 455.Google Scholar
Wesselink, A.J. (1947). B.A.N., 10, 256.Google Scholar
Wesselink, A.J. (1969). M.N.R.A.S., 144, 297.CrossRefGoogle Scholar