Category:
Journal Reprints
Sub-Category:
Astrophysics
Date Published:
April 2009
Keywords:
ballistic theory of Ritz (BTR), Ritz effect, Cepheids, Pulsars, Mössbauer effect, Copernicus
Filename:
Semikov_Variable Stars[trans]_19Apr(2009)1-7.pdf
Publication:
Proceedings of 2009 UNN Cosmoconference
Comments:
Translated to English with Google Translate by Thomas E. Miles
Abstract:
It has now been discovered that many physically variable stars are components of binary star systems. The variability of their brightness and spectrum is now associated with the rotation of these stars in orbit, around the axis. Thus, duality was discovered in new stars. It is even admitted that almost all novae are double [1, 2]. The movement of stars in an orbit (often highly elongated) with a periodic approach, it is believed, gives rise to their bright flares. One star, by its gravitation, causes disturbances in the atmosphere and interior of another, leading either to the explosion of the star from the imbalance of nuclear processes, or to the exchange of masses of stars, also accompanied by noticeable fluctuations in the brightness and spectrum of stars [1]. This is the generally accepted mechanism for new outbreaks. But taking into account the duality of novae makes it possible to propose a simpler flare mechanism associated with the Ritz effect.
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