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Short-Term Amplitude Variation of FM Com (=HR 4684)

  • M. Pararó (a1), J. Pena (a2), R. Peniche (a2), C. Ibanoglu (a3), Z. Tunca (a3) and S. Evren (a3)...
Abstract

Using unpublished data obtained in 1982 at Mexico and Turkey combined with Hungarian observations the process of amplitude variation of the frequency at 18.5 c/d is shown. The time scale of the amplitude increase is less than 100 days.

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References
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Breger, M., Garrido, R.. Lin, Huang, Shi-yang, Jiang, Zi-he, Guo. Frueh, M. and Pararó, M.: 1989, Astronomy and Astrophysics 214, 209.
Breger, M., McNamara, B.J., Kerschbaum, F., Lin, Huang, Shi-yang, Jiang, Zi-he, Guo and Poretti, E.: 1990, Astronomy and Astrophysics 231, 56.
Kovács, G. and Pararó, M.: 1989, Monthly Notices of the RAS 237, 201.
Kurtz, D.W.: 1980, Monthly Notices of the RAS 193, 61.
Paparó, M. and Kovács, G.: 1984, Astrophysics and Space Science 105, 357.
Stobie, R.S. and Shobbrook, R.R.: 1976, Monthly Notices of the RAS 174, 401.
Stobie, R.S., Pickup, D.A. and Shobbrook, R.R.: 1977, Monthly Notices of the RAS 179, 389.
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Proceedings of the International Astronomical Union
  • ISSN: -
  • EISSN: 0252-9211
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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