Analysis of the adiabatical pulsation of cepheids Report as inadecuate

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M.G. Corona-Galindo ; A.L. Gelover-Santiago ;Revista Mexicana de Física 2016, 62 (1)

Author: H. Dehnen



Revista Mexicana de Física ISSN: 0035-001X Sociedad Mexicana de Física A.C. México Dehnen, H.; Corona-Galindo, M.G.; Gelover-Santiago, A.L. Analysis of the adiabatical pulsation of Cepheids Revista Mexicana de Física, vol.
62, núm.
1, enero-febrero, 2016, pp.
20-30 Sociedad Mexicana de Física A.C. Distrito Federal, México Available in: How to cite Complete issue More information about this article Journals homepage in Scientific Information System Network of Scientific Journals from Latin America, the Caribbean, Spain and Portugal Non-profit academic project, developed under the open access initiative RESEARCH Revista Mexicana de Fı́sica 62 (2016) 20–30 JANUARY-FEBRUARY 2016 Analysis of the adiabatical pulsation of Cepheids H.
Dehnen Konstanz Universitaet, Fakultaet fuer Physik, Postfach 55 60, 7750 Konstanz, Germany, e-mail: M.G.
Corona-Galindo Instituto Nacional de Astrofı́sica,Óptica y Electrónica, Apartado Postal 216, 72840 Tonantzintla, Puebla, México, e-mail: A.L.
Gelover-Santiago Facultad de Ciencias, Universidad Nacional Autónoma de México, Circuito Exterior S-N, Ciudad Universitaria, México D.F.
04510, e-mail: Received 30 April 2015; accepted 13 October 2015 A model for the adiabatical pulsation of a Cepheid based on primary physical principles such as energy conservation, mechanical adiabaticity and hydrostatic equilibrium is presented.
The adiabatical treatment of the pulsation has been already studied by other authors but the novelty of our model is that it allows to obtain physical parameters of the star, namely the amplitude of the oscillation, the mass, maximal velocity of the pulsation and luminosity. Keywords: Geophysics; astronomy and astrophysics; stars; variable; peculiar stars; cepheids. PACS: 97.30.-d; 97.30.Gj 1.
Introduction In the present work we are principally ...

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