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20012008
most citedThe BOES spectropolarimeter for Zeeman measurements of stellar magnetic fields

103 citations · 233 across the 5 of their papers we have counts for

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astro-ph200841 cited

The pecular magnetic field morphology of the white dwarf WD 1953-011: evidence for a large-scale magnetic flux tube?

G. Valyavin, G. A. Wade, S. Bagnulo +4

We present and interpret new spectropolarimetric observations of the magnetic white dwarf WD 1953-011. Circular polarization and intensity spectra of the H spectral line demonst…

astro-ph200824 cited

Precise Radial Velocities of Polaris: Detection of Amplitude Growth

Byeong-Cheol Lee, David. E. Mkrtichian, Inwoo Han +2

We present a first results from a long-term program of a radial velocity study of Cepheid Polaris (F7 Ib) aimed to find amplitude and period of pulsations and nature of secondary p…

astro-ph2007103 cited

The BOES spectropolarimeter for Zeeman measurements of stellar magnetic fields

Kang-Min Kim, Inwoo Han, Gennady G. Valyavin +9

We introduce a new polarimeter installed on the high-resolution fiber-fed echelle spectrograph (called BOES) of the 1.8-m telescope at the Bohyunsan Optical Astronomy Observatory,…

astro-ph200621 cited

The Lorentz force in atmospheres of CP stars: Aurigae

D. Shulyak, G. Valyavin, O. Kochukhov +7

Several dynamical processes may induce considerable electric currents in the atmospheres of magnetic chemically peculiar (CP) stars. The Lorentz force, which results from the inter…

astro-ph200644 cited

A search for kilogauss magnetic fields in white dwarfs and hot subdwarf stars

G. Valyavin, S. Bagnulo, S. Fabrika +4

We present new results of a survey for weak magnetic fields among DA white dwarfs with inclusion of some brighter hot subdwarf stars. We have detected variable circular polarizatio…

astro-ph2001

An Upper Limit to the Mass of rho1 Cnc's Radial Velocity Companion

Melissa A. McGrath, Edmund Nelan, David C. Black +7

Doppler spectroscopy of rho1 Cnc has detected evidence of a companion with an orbital period of 14.65 days and a minimum mass of 0.88 Jupiter masses. Astrometric observations perfo…