most citedThe origin of hydrogen line emission for five Herbig Ae/Be stars spatially resolved by VLTI/AMBER spectro-interferometry

157 citations · 384 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR20098 cited

A new spectroscopic and interferometric study of the young stellar object V645 Cyg

A. S. Miroshnichenko, K. -H. Hofmann, D. Schertl +14

We present the results of high-resolution optical spectroscopy, low-resolution near-IR spectroscopy and near-infrared speckle interferometry of the massive young stellar object can…

astro-ph.SR2009117 cited

Tracing the young massive high-eccentricity binary system Theta 1 Orionis C through periastron passage

S. Kraus, G. Weigelt, Y. Y. Balega +10

The nearby high-mass star binary system Theta 1 Orionis C is the brightest and most massive of the Trapezium OB stars at the core of the Orion Nebula Cluster, and it represents a p…

astro-ph2008157 cited

The origin of hydrogen line emission for five Herbig Ae/Be stars spatially resolved by VLTI/AMBER spectro-interferometry

S. Kraus, K. -H. Hofmann, M. Benisty +14

To trace the accretion and outflow processes around YSOs, diagnostic spectral lines such as the BrG 2.166 micron line are widely used, although due to a lack of spatial resolution,…

astro-ph20088 cited

AMBER closure and differential phases: accuracy and calibration with a Beam Commutation

Florentin Millour, Romain Petrov, Martin Vannier +1

The first astrophysical results of the VLTI focal instrument AMBER have shown the importance of the differential and closure phase measures, which are supposed to be much less sens…

astro-ph200844 cited

Spatially resolving the hot CO around the young Be star 51 Ophiuchi

E. Tatulli, F. Malbet, F. Menard +6

51 Oph is one of the few young Be stars displaying a strong CO overtone emission at 2.3 microns in addition to the near infrared excess commonly observed in this type of stars. In…

astro-ph200810 cited

First VLTI infrared spectro-interferometry on GCIRS 7 - Characterizing the prime reference source for Galactic center observations at highest angular resolution

J. -U. Pott, A. Eckart, A. Glindemann +5

Investigating the environment of the massive black hole SgrA* at the center of the Galaxy requires the highest angular resolution available to avoid source confusion and to study t…