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most citedThe BOES spectropolarimeter for Zeeman measurements of stellar magnetic fields

103 citations · 871 across the 43 of their papers we have counts for

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astro-ph2008★ 29 cited

Rotation and surface abundance peculiarities in A-type stars

Yoichi Takeda, Inwoo Han, Dong-Il Kang +2

In an attempt of clarifying the connection between the photospheric abundance anomalies and the stellar rotation as well as of exploring the nature of "normal A" stars, the abundan…

astro-ph2008★ 41 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-ph2008★ 24 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-ph2007★ 103 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-ph2006★ 21 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-ph2006★ 44 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…