Publications on long period pulsating (Mira and SR) stars at JATE University, Szeged, Hungary
- 1. Szatmáry K., Mizser A., Dömény G.: 1985, Multiple-period
- red variables: Y Lyncis and W Cygni,
- BAA Variable Star Section Circular No.62. 2-8.
- 2. Szatmáry K.: 1986, Semiregular red variable stars - a field of
- cooperation between amateurs and professionals,
- Proc. GIREP '86 Conference, Copenhagen, Denmark
- ESA SP-253 p.407-409.
- 3. Mizser A., Szatmáry K., Tepliczky I.: 1990, Some results of
- Hungarian variable star observers,
- "First European Meeting of the AAVSO" Brussels,
- Journal of AAVSO 19. No.1. 47-51.
- 4. Szatmáry K.: 1990, Pulsating variable stars in binary systems,
- "First European Meeting of the AAVSO" Brussels,
- Journal of AAVSO 19. No.1. 52-56.
- 5. Szatmáry K., Gál J.: 1992, Wavelet analysis of some pulsating stars,
- In: Inside the Stars, IAU Colloquium No. 137, Vienna,
- Austria, Communications in Astroseismology No.43. 8/19.
- Astron.Soc.Pac.Conf.Ser. Vol.40. 761-763. 1993
- Eds. W.W.Weiss and A.Baglin
- 6. Szatmáry K., Vinkó J.: 1992, Periodicities of the light curve
- of the semiregular variable star Y Lyncis,
- Monthly Notices Royal Astron. Soc. 256, 321-328.
- 7. Gál J., Szatmáry K.: 1993, Search for period changes of semiregular
- variable stars with wavelet analysis,
- Proc. Conference on "Applications of Time Series
- Analysis in Astronomy and Meteorology" ed. O. Lessi,
- pp. 191-194. Padova, Italy, 1993
- 8. Kiss L.L.: 1994, Light Curves of Variable Stars for 1988-1992,
- Publ. of Hungarian Astronomical Association
- 9. Szatmáry K.: 1994, Wavelet analysis of deficient and gapped data
- series of variable stars, Proc. 22nd IAU General Assembly,
- Hague, Netherland
- Astronomy Posters, Abstracts, Ed. Hugo van Woerden, p.251
- 10. Gál J., Szatmáry K.: 1995, T Ursae Minoris: A Mira star with rapidly
- decreasing period, Astronomy and Astrophysics 297, 461-464.
- 11. Gál J., Szatmáry K.: 1995, Period update of 40 Mira stars,
- Astrophysics and Space Science 225, 101-106.
- 12. Szatmáry K., Gál J., Kiss L.L.: 1995, Light curve analysis of long
- period pulsating stars with the wavelet method: The
- semiregular star V Boo, Proc. IAU Coll. 155
- "Astrophysical Applications of Stellar Pulsation"
- Astron. Soc. Pac. Conf. Ser. Vol.83. 417-418. 1995
- eds. R.S. Stobie and P.A. Whitelock, Cape Town, South Africa
- 13. Gál J., Szatmáry K.: 1995, Mode switching in red semiregular variable
- stars?, Proc. IAU Coll. 155 "Astrophysical Applications
- of Stellar Pulsation"
- Astron. Soc. Pac. Conf. Ser. Vol.83. 405-406. 1995
- eds. R.S. Stobie and P.A. Whitelock, Cape Town, South Africa
- 14. Gál J., Szatmáry K.: 1995, Multiperiodicity in red semiregular
- variables, poster on IAU Coll. 155 "Astrophysical
- Applications of Stellar Pulsation" Cape Town, South Africa
- 15. Szatmáry K., Gál J., Kiss L.L.: 1996, Applications of wavelet analysis
- in variable star research. II. The semiregular star V Bootis,
- Astronomy and Astrophysics 308, 791-798.
- 16. Szatmáry K., Kiss L.L.: 1996, The strange semiregular star 89 Her,
- poster on IAPPP Symposium '96 Baja, Hungary
- 17. Szatmáry K.: 1997, Amplitude and period changes in the light variations
- of some Mira and SR stars,
- poster on 23rd IAU General Assembly, Kyoto, Japan
- Abstract Book, JD24-021P, p.128.
- 18. Szatmáry K.: 1998, Amplitude and period changes in the light variations
- of some SR stars,
- Pulsating Stars - Recent Developments in Theory and
- Observation, Proceedings of Joint Discussion No. 24
- of the 23rd General Assembly of the IAU, Kyoto, Japan
- pp. 103-106, Eds. M. Takeuti and D.D. Sasselov,
- Universal Academy Press, Japan
- 19. Kiss L.L.: 1998, Present Activities of the Hungarian Astronomical
- Association - Variable Star Section, Proc. of the II. European
- Meeting of the AAVSO Sion, Switzerland, ASP Conf. Series, in press
- 20. Szatmáry K., Kiss L.L.: 1998, Multiperiodicity in semiregular
variables,
- C2-02 contributed talk on IAU Symposium No.191 "Asymptotic
- Giant Branch Stars", Montpellier, France, Aug 1998,
- Abstract Booklet p.49