most citedOscillations in Procyon A: First results from a multi-site campaign

3 citations · 3 across the 1 of their papers we have counts for

collaborators

6 papers

astro-ph2008158 cited

A multi-site campaign to measure solar-like oscillations in Procyon. I. Observations, Data Reduction and Slow Variations

Torben Arentoft, Hans Kjeldsen, Timothy R. Bedding +45

We have carried out a multi-site campaign to measure oscillations in the F5 star Procyon A. We obtained high-precision velocity observations over more than three weeks with eleven…

astro-ph200816 cited

Evidence for a companion to BM Gem, a silicate carbon star

Hideyuki Izumiura, Kunio Noguchi, Wako Aoki +12

Balmer and Paschen continuum emission as well as Balmer series lines of P Cygni-type profile from H_gamma through H_23 are revealed in the violet spectra of BM Gem, a carbon star a…

astro-ph20073 cited

Oscillations in Procyon A: First results from a multi-site campaign

S. Hekker, T. Arentoft, H. Kjeldsen +45

Procyon A is a bright F5IV star in a binary system. Although the distance, mass and angular diameter of this star are all known with high precision, the exact evolutionary state is…

astro-ph200779 cited

A Substellar Companion to the Intermediate-Mass Giant 11 Com

Y. J. Liu, Bun'ei Sato, G. Zhao +16

We report the detection of a substellar companion orbiting the intermediate-mass giant star 11 Com (G8 III). Precise Doppler measurements of the star from Xinglong station and Okay…

astro-ph2004

Spectroscopic Studies of Extremely Metal-Poor Stars with Subaru/HDS:I. Observational Data

S. Honda, W. Aoki, H. Ando +14

We have obtained high-resolution (R 50,000 or 90,000), high-quality (S/N $\ga$ 100) spectra of 22 very metal-poor stars ([Fe/H] $\la$ -2.5) with the High Dispersion Spectr…

astro-ph2003

2MASSJ0516288+260738: Discovery of the first eclipsing late K + Brown dwarf system?

S. L. Schuh, G. Handler, H. Drechsel +22

We report the discovery of a new eclipsing system less than one arcminute south of the pulsating DB white dwarf KUV 05134+2605. The object could be identified with the point source…