Evolution of the optical and hard X-ray activity of AM Her in a season dominated by the high states

0463124 - ASÚ 2017 RIV NL eng J - Journal Article
Šimon, Vojtěch
Evolution of the optical and hard X-ray activity of AM Her in a season dominated by the high states.
Astrophysics and Space Science. Roč. 361, č. 7 (2016), 235/1-235/8. ISSN 0004-640X. E-ISSN 1572-946X
Grant - others:GAO(CZ) GC13-39464J
Institutional support: RVO:67985815
Keywords : X-rays binaries * cataclysmic variables * radiation mechanisms
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
Impact factor: 1.622, year: 2016

The long-term activity of AM Her, the prototype of polars, consists of interchanging high and low states. This analysis uses the data from the BAT/Swift, MAXI/ISS, and AAVSO data archives (including long CCD V-band night series) for investigating the relation of the time evolution of intensities in the hard X-ray, medium/hard X-ray, and the optical bands on super-orbital timescale in a season dominated by the long high-state episodes. The observations mapped the relation of the cyclotron and bremsstrahlung luminosities in such episodes. Although an increase of intensity of the cyclotron emission is generally accompanied by a brightening of the bremsstrahlung component, this relation differs for the individual high-state episodes. These variations were accompanied by the large changes of the optical modulation. In my view, all of these variations suggest variations of the dimensions and structure of the cyclotron emitting region(s), not only the changes of the mass accretion rate. The activity during a decline (much less steep than the state transition) from an initial very bright peak can be explained by a gradual evolution of the conditions in stratified shock regions in a single high state episode. The observed behavior in the neighboring high-state episodes is also important for explaining the mechanisms which cause the low state between them. In the interpretation, some low-state episodes cause that AM Her develops a different accretion mode than the one before entering the low state. Each high-state episode is a complex phenomenon in the history of accretion in this system.
Permanent Link: http://hdl.handle.net/11104/0262403