DOI: https://doi.org/10.18524/1810-4215.2013.26.81903

T CEP, U UMI, Z SCO – MIRA-TYPE VARIABLES WITH CYCLIC PERIOD CHANGES

V. I. Marsakova

Анотація


Period and amplitude changes of three Mira-type variables have been analyzed. Characteristics of  long-term cyclicity were obtained

Ключові слова


Stars; LPVs; Mira-type; period changes; individual; T Cep; U UMi; Z Sco

Повний текст:

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Посилання


Andronov I.L.: 1997, Astron. Astrophys. Suppl., 125, 207

Andronov I.L., Baklanov A.V.: 2004, Astronomy School Reports, 5, 264, http://uavso.pochta.ru/mcv

Andronov I. L.:2005, ASP Conference Series, 335, 37°

Andronov I.L., Marsakova V.I.: 2006, Astrophysics, 49, 370.

Kudashkina L. S., Rudnitskij G. M.: 1995, Odessa Astron. Publ., 7, 63.

Marsakova V.I., Andronov I.L.: 1997, Kinematics and Physics of Celestial Bodies, 13, № 6, 49.

Marsakova V.I., Andronov I.L.: 2000, ASP Conference Series, 203, 131.

Marsakova V.I.: 1999, Odessa Astronomical Publication, 12,

Marsakova V.I., Andronov I.L: 2006, Astrophysics, 49, 506.

Marsakova V.I., Andronov I.L.: 2007, Astrophysics, 50, 99.

Samus N.N., Durlevich O.V., Kazarovets E V., Kireeva N.N., Pastukhova E.N., Zharova A.V., et al.: 2012, General Catalog of Variable Stars (GCVS database, Version 2012Jan), http://www.sai.msu.su/gcvs/gcvs/

Zijlstra A.A. & Bedding T.R.: 2002, Journal AAVSO, 31, 2.




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