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The Formation of Absorption Lines in a Moving Atmosphere

S. Chandrasekhar

S. Chandrasekhar

  • Yerkes Observatory of the University of Chicago, Williams Bay, Wisconsin

Rev. Mod. Phys. 17, 138 – Published 1 April, 1945

DOI: https://doi.org/10.1103/RevModPhys.17.138

References (10)

  1. O. Struve, Astrophys. J. 98, 98 (1943) W. Hiltner, 99, 103 (1944) P. W. Merrill and R. Sanford, 100, 14 (1944)
  2. W. H. McCrea and K. K. Mitra, Zeits. f. Astrophys. 11, 359 (1936)
  3. S. Chandrasekhar, Astrophys. J. 100, 76, 117 (1944) ibid.101, 95, 328, 348 (1945)
  4. A. Schuster, Astrophys. J. 21, 1 (1905)
  5. A. G. Webster, Partial differential equations of mathematical physics (1933), Section 46, p. 173
  6. Webster, reference 5, pp. 160-188 and 239-255 P. Frank and R. von Mises, Die Differential und Integralgleichungen der Mechanik und Physik (Rosenberg, New York, 1943), Vol. I, pp. 779-817
  7. G. N. Watson, Theory of Bessel Functions (Cambridge University Press, England, 1944), p. 393
  8. G. N. Watson, Theory of Bessel Functions (Cambridge University Press, England, 1944), p. 141
  9. Omitted endnote

  10. G. N. Watsonthe British Association Mathematical Tables, VI: Bessel functions of order zero and unity (Cambridge University Press, England, 1937)

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