A Historical Sketch of the Beat Cepheid Studies

Author:

Petersen Jørgen Otzen,Takeuti Mine

Publisher

Springer Netherlands

Reference84 articles.

1. Alcock, C., Allsman, R. A., Axelrod, T. S., et al. (The MACHO Collaboration) (1995). The MACHO Project LMC Variable Star Inventory. I. Beat Cepheids–Conclusive Evidence for the Excitation of the Second Overtone in Classical Cepheids. Astron. J., 109: 1653–1662.

2. Alcock, C., Allsman, R. A., Axelrod, T. S., et al. (The MACHO Collaboration) (1999). The MACHO Project LMC Variable Star Inventory. VI. The Second Overtone Mode of Cepheid Pulsation from First/Second Overtone Beat Cepheids. Astrophys. J., 511: 185–192.

3. Andreasen, G. K., and Petersen, J. O. (1988). Double Mode Pulsating Stars and Opacity Changes. Astron. Astrophys. (Letters), 192: L4 - L6.

4. Antonello, E., Carcano, P., and Kanbur, S. M. (1997). On the Masses and Luminosities of Double-mode Cepheids. Astron. Astrophys., 319: 863–866.

5. Antonello, E., and Poretti, E. (1986). Structural Properties of the Light Curves of s-Cepheids. Astron. Astrophys., 169: 149–153.

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