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Prog. Theor. Phys. Vol. 46 No. 5 (1971) pp. 1627-1628

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Letters

Contribution to the Helium Content of the Galaxy from Pulsationally Unstable Stars Evolving Inhomogeneously

Yasuo Tanaka and Shiro Sakashita^*

Faculty of Education, Ibaraki University, Mito
^*Department of Physics, Hokkaido University, Sapporo

(Received July 6, 1971)

URL : http://ptp.ipap.jp/link?PTP/46/1627/
DOI : 10.1143/PTP.46.1627

References:

R. J. Tayler, Quart. J. R. Astron. Soc. 8 (1967), 313.
J. W. Truran, C. J. Hansen and A. G. W. Cameron, Can. J. Phys. 43 (1965), 1916.
G. Burbidge, P. A. S. P. 70 (1958), 83.
P. Ledoux, Observatory, No. 960 (1967), 207.
A. Ferrari, R. Callino and A. Massani, Astron. Astrophys. 10 (1971), 481.
Y. Tanaka, unpublished (1967).
A. Boury, Ann. Ap. 26 (1963), 354.

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