activity
19962019
most citedFirst Light for GRAVITY: Phase Referencing Optical Interferometry for the Very Large Telescope Interferometer

588 citations · 1.3k across the 22 of their papers we have counts for

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11 papers · 1 filter

astro-ph2007

A study of the magnetic helium variable emission-line star HD 125823

S. Hubrig, N. Nesvacil, F. Gonzalez +2

The 5.9 M_sun star HD 125823 is a striking helium variable with a period of 8.82 d, ranging in helium spectral type from He-strong B2 to He-weak B8. For the first time we present h…

astro-ph2007★ 23 cited

Heavy Calcium in CP Stars

C. R. Cowley, S. Hubrig, F. Castelli +2

Large wavelength shifts of infrared triplet lines of Ca II have been observed in the spectra of HgMn and magnetic Ap stars. They have been attributed to the heavy calcium isotopes,…

astro-ph2006★ 29 cited

Tests of stellar model atmospheres by optical interferometry IV: VINCI interferometry and UVES spectroscopy of Menkar

M. Wittkowski, J. P. Aufdenberg, T. Driebe +3

We present K-band interferometric and optical spectroscopic observations of Menkar obtained with the instruments VINCI and UVES at Paranal Observatory. Spherically symmetric PHOENI…

astro-ph2006★ 64 cited

Inhomogeneous surface distribution of chemical elements in the eclipsing binary AR Aur: A new challenge for our understanding of HgMn stars

S. Hubrig, J. F. Gonzalez, I. Savanov +4

We present the results of a high spectral resolution study of the eclipsing binary AR Aur. AR Aur is the only known eclipsing binary with a HgMn primary star exactly on the ZAMS an…

astro-ph2005★ 112 cited

Li in NGC 6752 and the formation of globular clusters

L. Pasquini, P. Bonifacio, P. Molaro +5

Li abundances for 9 Turnoff (TO) stars of the intermediate metallicity cluster ([Fe/H]=-1.4) NGC6752 are presented. The cluster is known to show abundance anomalies and anticorrela…

astro-ph2004★ 79 cited

Magnetic fields in Herbig Ae stars

S. Hubrig, M. Schoeller, R. V. Yudin

Herbig Ae stars are young A-type stars in the pre-main sequence evolutionary phase with masses of ~1.5-3 M_o. They show rather intense surface activity (Dunkin et al. 1997) and inf…

astro-ph2003★ 21 cited

A Possible New Transiting Planet

S. Dreizler, P. Hauschildt, W. Kley +4

Recently, 59 low-luminosity object transits were reported from the Optical Gravitational Lensing Experiment (OGLE). Our follow-up low-resolution spectroscopy of 16 candidates provi…

astro-ph2002★ 73 cited

Element abundances in cool white dwarfs. II. Ultraviolet observations of DZ white dwarfs

B. Wolff, D. Koester, J. Liebert

We present a small data base of homogeneously derived photospheric element abundances of DZ white dwarfs and related objects. Our previous investigations are supplemented with the…

astro-ph2001★ 37 cited

Equilibrium abundances in hot DA white dwarfs as derived from self-consistent diffusion models I. Analysis of spectroscopic EUVE data

S. L. Schuh, S. Dreizler, B. Wolff

We present the first analysis of an EUV selected sample of hot DA white dwarfs using a new type of atmospheric models. These models take into account the interplay between gravitat…

astro-ph2001★ 23 cited

FUSE observations of hot white dwarfs

B. Wolff, J. W. Kruk, D. Koester +3

We have analyzed FUSE observations of six hot white dwarf stars: four DA white dwarfs with T_eff >= 45000K, the DAO Feige55 (T_eff = 55000K), and the DA CD -38 10980 (T_eff = 24000…

astro-ph1996★ 1 cited

Extragalactic symbiotic systems --- IV. The supersoft X-ray source SMC 3

Stefan Jordan, Werner Schmutz, Burkhard Wolff +2

We present a consistent model for the UV and supersoft X-ray emission from the symbiotic nova SMC3 (=RX J0048.4-7332). Following the present picture of symbiotic stars, the model c…