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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.
Abstract
Via simultaneous multicolor photometry and polarimetry of AM Herculis, we find correlations among polarization, flux, and color in the V and I bands in periodic and nonperiodic (i.e., flickering) activity. The primary minimum observed in both bands is accompanied by a blueward shift of the (B - R) color and a decrease in the absolute value of the percent circular polarization in the V band. Outside primary minimum, peaks of flickering activity tend to be associated with an increase in the absolute value of the circular polarization and the concurrent reddening of the (B - R) and (R - I) colors. The visual light curve of AM Her can be explained by a flickering, circularly polarized light source which is obscured at primary minimum, and is redder than the total system color in the URVRI bands.

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Book ChapterDOI

The AM Herculis Magnetic Variables

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.
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