Journal ArticleDOI
Correlated photometric and polarimetric phenomena in AM Herculis
TLDR
In this article, a multicolor photometry and polarimetry of AM Herculis was used to find correlations among polarization, flux, and color in the V and I bands in periodic and non-periodic (i.e., flickering) activity.Citations
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Book ChapterDOI
The AM Herculis Magnetic Variables
James Liebert,H. S. Stockman +1 more
TL;DR: The observational properties of the ten known AM Her systems are reviewed in this article, where the important physical processes involved in the accretion flow and funnel shock, with emphasis on the properties of emission line regions, are discussed.
Journal ArticleDOI
Low-State Flaring Events in AM Herculis
TL;DR: In this paper, a photometric monitoring campaign has been conducted in order to investigate the character and origin of flaring events occasionally seen in the long-term low-state light curve of the polar prototype AM Her.
Journal ArticleDOI
The system AM Her = 4U 1814 + 50
TL;DR: The binary system AM Herculis = 4U 1814 + 50 gives the first well ascertained example of an X-ray emitting magnetic white dwarf as mentioned in this paper, whose orbital period (3.1h) is apparent from X-rays to IR frequencies and in linear and circular polarization.
Journal ArticleDOI
Updated photometry and orbital period analysis for the polar am herculis on the upper edge of the period gap
TL;DR: In this paper, three plausible mechanisms-spot motion, the light travel-time effect, and magnetic active cycles-were discussed in detail, in order to explain the prominent periodic modulation.
Journal ArticleDOI
On the mechanism of the “Noisar” phenomenon in magnetic close binary systems
TL;DR: In this article, the authors discuss the mechanisms of the noise phenomenon in AM Herculis-type stars and show that the instability of some types may be excited, such as axi-symmetrical quasi-periodical penetration of the low-density "bulks" from the column axis to the outer parts, boiling, and switching of the accretion from one half of the polar cap to another and vice versa.