134 citations · 385 across the 9 of their papers we have counts for
9 papers
Regularized 3D spectroscopy with CubeFit: method and application to the Galactic Center Circumnuclear disk
Thibaut Paumard, Anna Ciurlo, Mark R. Morris +2
The Galactic Center black hole and the nuclear star cluster are surrounded by a clumpy ring of gas and dust (the circumnuclear disk, CND) that rotates about them at a standoff dist…
Clumpiness of the interstellar medium in the central parsec of the Galaxy from H2 flux extinction correlation
Anna Ciurlo, Thibaut Paumard, Daniel Rouan +1
The central parsec of the Galaxy contains a young star cluster embedded in a complex interstellar medium. The latter mainly consists of a torus of dense clumps and streams of molec…
Hot molecular hydrogen in the central parsec of the Galaxy through near-infrared 3D fitting
Anna Ciurlo, Thibaut Paumard, Daniel Rouan +1
Aims. We have investigated neutral gas in the central cavity of the circumnuclear disk (CND) at the Galactic Center, where the ionized minispiral lies, to describe the H2 distribut…
Future mmVLBI Research with ALMA: A European vision
R. P. J. Tilanus, T. P. Krichbaum, J. A. Zensus +165
Very long baseline interferometry at millimetre/submillimetre wavelengths (mmVLBI) offers the highest achievable spatial resolution at any wavelength in astronomy. The anticipated…
Massive Young Stars in the Galactic Center
H. Bartko
We summarize our latest observations of the nuclear star cluster in the central parsec of the Galaxy with the adaptive optics assisted, integral field spectrograph SINFONI on the E…
Star formation in the central 0.5 pc of the Milky Way
Thibaut Paumard
The supermassive black hole candidate at the Galactic Center is surrounded by a parsec-scale star cluster, which contains a number of early type stars. The presence of such stars h…
Kinematic and structural analysis of the Minispiral in the Galactic Center from BEAR spectro-imagery
Thibaut Paumard, Jean-Pierre Maillard, Mark Morris
Integral field spectroscopy of the inner region of the Galactic Center, over a field of roughly 40"x40" was obtained at 2.06 microns (He I) and 2.16 microns (Brackett-gamma) using…
The nature of the Galactic Center source IRS 13 revealed by high spatial resolution in the infrared
J. P. Maillard, T. Paumard, S. R. Stolovy +1
High spatial resolution observations in the 1 to 3.5 micron region of the Galactic Center source known historically as IRS 13 are presented. They include ground-based adaptive opti…
New Results on the Helium Stars in the Galactic Center Using BEAR Spectro-Imagery
T. Paumard, J. P. Maillard, M. Morris +1
Integral field spectroscopy of the central parsec of the Galactic Center was obtained at 2.06 microns using BEAR, an imaging Fourier Transform Spectrometer, at a spectral resolutio…