Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...254..232l&link_type=abstract
Astrophysical Journal, Part 1, vol. 254, Mar. 1, 1982, p. 232-241.
Astronomy and Astrophysics
Astrophysics
27
Binary Stars, Circular Polarization, Magnetic Stars, Stellar Magnitude, Stellar Spectrophotometry, Constellations, Cyclotron Radiation, Ephemerides, H Alpha Line, H Beta Line, Harmonic Radiation, Interstellar Extinction, Light Curve, Mass Transfer, Polarimetry, Visual Photometry
Scientific paper
Spectrophotometry, photometry, and circular polarimetry are reported of the magnetic binary AN UMa during February/March 1979, when it reached a very low state of B (approximately 19-20), 2 mag fainter than ever observed previously. The B light curve was generally similar in shape to that for the high state, although only approximately 0.6 of a period was covered. The energy distribution became markedly redder compared with that in higher states; the I magnitude had dropped only to about 17. The low-state I-band circular polarization reached a peak value of -35%, which is considerably stronger than in the high state; the presumed cyclotron funnel source thus remained dominant, at least at red wavelengths. The spectrophotometry at V approximately 17.5-18.5 revealed a red continuous energy distribution; there was weak H-alpha emission, a probable very broad emission feature near H-beta, but no evidence for strong absorption features from the secondary or magnetic primary.
Bond Howard E.
Grauer Albert D.
Liebert James
Tapia Saul
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