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Magnetic field measurements on four yellow supergiants. I
Authors:S I Plachinda
Institution:(1) Crimean Astrophysical Observatory, Ukraine
Abstract:Multiyear high precision measurements of the longitudinal component of the magnetic field (Be) of four supergiants are reported: betaAqr (G0 Ib), agrAqr (G2 Ib), epsivGem (G8 Ib), and epsivPeg (K2 Ib). The best measurement accuracy, sgr=0.8 G, was achieved for epsivPeg. A Monte Carlo method was used to test the reliability of the derived measurement errors. The differences between the observational errors and the calculated Monte Carlo errors were sim3.2%. For betaAqr and agrAqr no statistically significant value of the magnetic field was recorded when averaged over a night. For eGem the following overnight average values of the magnetic field were recorded on five nights: 11.1±2.7 G, 9.8±2.5 G, –10.5±3.0 G, 38.1±7.4 G, and 5.3±1.5 G. For epsivPeg the magnetic field recorded over two nights was –5.3±0.9 G and – 2.7±0.8 G.Translated from Astrofizika, Vol. 48, No. 1, pp. 15–28 (February 2005).
Keywords:stars  activity  magnetic field —  stars  individual  betaAqr" target="_blank">gif" alt="beta" align="MIDDLE" BORDER="0">Aqr  agrAqr" target="_blank">gif" alt="agr" align="BASELINE" BORDER="0">Aqr  epsivGem" target="_blank">gif" alt="epsiv" align="BASELINE" BORDER="0">Gem  epsivPeg" target="_blank">gif" alt="epsiv" align="BASELINE" BORDER="0">Peg
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