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19982025
most citedThe dusty torus in the Circinus galaxy: a dense disk and the torus funnel

216 citations · 1.4k across the 39 of their papers we have counts for

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15 papers · 1 filter

astro-ph2008★ 20 cited

Discovery of a strong Baldwin effect in mid-infrared AGN lines

S. F. Hoenig, A. Smette, T. Beckert +5

We present the discovery of a Baldwin effect in 8 nearby Seyfert galaxies for the three most prominent mid-infrared forbidden emission lines observable from the ground that are com…

astro-ph2006★ 4 cited

First astrophysical results from AMBER/VLTI

Fabien Malbet, Romain G. Petrov, Gerd Weigelt +5

The AMBER instrument installed at the Very Large Telescope (VLT) combines three beams from as many telescopes to produce spectrally dispersed fringes from milli-arcsecond angular s…

astro-ph2006★ 50 cited

Outflows from the high-mass protostars NGC 7538 IRS1/2 observed with bispectrum speckle interferometry -- Signatures of flow precession

S. Kraus, Y. Balega, M. Elitzur +6

NGC 7538 IRS1 is a high-mass (approx. 30 M_sun) protostar with a CO outflow, an associated UCHII region, and a linear methanol maser structure, which might trace a Keplerian-rotati…

astro-ph2005★ 2 cited

First AMBER/VLTI observations of hot massive stars

R. G. Petrov, F. Millour, O. Chesneau +45

AMBER is the first near infrared focal instrument of the VLTI. It combines three telescopes and produces spectrally resolved interferometric measures. This paper discusses some pre…

astro-ph2002★ 19 cited

UBVJHKLM photometry and modeling of R Coronae Borealis

B. F. Yudin, J. D. Fernie, N. R. Ikhsanov +2

We present the results of UBVJHKLM photometry of R CrB spanning the period from 1976 to 2001. Studies of the optical light curve have shown no evidence of any stable harmonics in t…

astro-ph2002

Spectral Observations of Stars in Late Stages of Stellar Evolution

T. Bloecker, K. -H. Hofmann, G. Weigelt

Interferometric observations of stars in late stages of stellar evolution and the impact of VLTI observations are discussed. Special attention is paid to the spectral information t…