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Time-Series Monitoring of Variable Stars in the Field of NGC7789

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Abstract

Through the photometric observations of NGC7789 with the Schmidt telescopefor four consecutive nights, sixteen variable stars were discovered. It was found that three are Algol (EA) type, seven are W UMa (EW) orβ Lyrae (EB) type and one is δ Scuti type.

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References

  • Bartholdi, P., Burnet, M. and Rufener, F.: 1984, Astron. Astrophys. 134, 120.

    Google Scholar 

  • Burbidge, E.M. and Sandage, A.: 1958, Astrophys. J. 128, 174.

    Article  ADS  Google Scholar 

  • Friel, E.D. and Janes, K.A.: 1993, Astron. Astrophys. 267, 75.

    ADS  Google Scholar 

  • Jahn, K., Kaluzny, J. and Rucinski, S.M.: 1995, Astron. Astrophys. 295, 101.

    ADS  Google Scholar 

  • McNamara, B.J. and Solomon, S.: 1981, Astron. Astrophys. Suppl. 43, 337.

    ADS  Google Scholar 

  • Park, N.K. and Nemec, J.M.: 1998, in preparation.

  • Pilachowski, C.A.: 1985, Publ. Astron. Soc. Pacific 97, 801.

    Article  ADS  Google Scholar 

  • Sperl, M.: 1998, unpublished.

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Kim, C., Park, NK. Time-Series Monitoring of Variable Stars in the Field of NGC7789. Astrophysics and Space Science 268, 387–396 (1999). https://doi.org/10.1023/A:1002046802785

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