Photometry and polarimetry of AM Herculis

Details Photometry and polarimetry of AM Herculis Photometry and polarimetry of AM Herculis

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.183p..73b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 183, June 1978, p. 73P-77P.

Astronomy and Astrophysics

Astronomy

3

Astronomical Photometry, Binary Stars, Magnetic Stars, Polarimetry, Autocorrelation, Fourier Analysis, Light Curve, Linear Polarization, Polarization Characteristics, Stellar Magnitude

Scientific paper

Some new high-speed photometric and polarimetric observations of AM Herculis are presented. These new data obtained during 1977 with the 2.5-m Isaac Newton telescope are compared to previous observations. Several properties are noted to have changed, in particular the size and structure of the periodic linear-polarization events. There is no evidence for periodic variation of the polarization apart from the 3-hr orbital period.

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