activity
19952026
most citedFrom filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

1.5k citations · 38.1k across the 501 of their papers we have counts for

collaborators
Showing 2005 · astro-phShow all

13 papers · 2 filters

astro-ph2005★ 21 cited

The IMF and Star Formation History of the Stellar Clusters in the Vela D Cloud

Fabrizio Massi, Leonardo Testi, Leonardo Vanzi

We present the results of a Near-Infrared deep photometric survey of a sample of six embedded star clusters in the Vela-D molecular cloud, all associated with luminous (~10^3 Lsun)…

astro-ph2005★ 34 cited

Exploring the Lower Mass Function in the young open Cluster IC 4665

W. J. de Wit, J. Bouvier, F. Palla +8

We present a study of the young (30-100Myr) open cluster IC 4665 with the aim to determine the shape of the mass function well into the brown dwarf regime. We photometrically selec…

astro-ph2005★ 136 cited

Search for massive protostar candidates in the southern hemisphere: II. Dust continuum emission

Maria T. Beltran, Jan Brand, Riccardo Cesaroni +4

In an ongoing effort to identify and study high-mass protostellar candidates we have observed in various tracers a sample of 235 sources selected from the IRAS Point Source Catalog…

astro-ph2005★ 96 cited

Disk and wind interaction in the young stellar object MWC 297 spatially resolved with VLTI/AMBER

F. Malbet, M. Benisty, W. J. De Wit +15

The young stellar object MWC 297 has been observed with the VLT interferometer equipped with the AMBER instrument. MWC 297 has been spatially resolved in the continuum with a visib…

astro-ph2005★ 33 cited

First results from a VLBA proper motion survey of H2O masers in low-mass YSOs: the Serpens core and RNO15-FIR

L. Moscadelli, L. Testi, R. S. Furuya +4

This article reports first results of a long-term observational program aimed to study the earliest evolution of jet/disk systems in low-mass YSOs by means of VLBI observations of…

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-ph2005★ 1 cited

VITRUV - Science Cases

Paulo J. V. Garcia, Jean-Phillipe Berger, Romano Corradi +11

VITRUV is a second generation spectro-imager for the PRIMA enabled Very Large Telescope Interferometer. By combining simultaneously up to 8 telescopes VITRUV makes the VLTI up to 6…

astro-ph2005

Disentangling the wind and the disk in the close surrounding of the young stellar object MWC297 with AMBER/VLTI

Fabien Malbet, M. Benisty, W. J. De Wit +13

The young stellar object MWC297 is a B1.5Ve star exhibiting strong hydrogen emission lines. This object has been observed by the AMBER/VLTI instrument in 2-telescope mode in a sub-…

astro-ph2005★ 157 cited

A resolved outflow of matter from a Brown Dwarf

Emma T. Whelan, Thomas P. Ray, Francesca Bacciotti +3

The birth of stars involves not only accretion but also, counter-intuitively, the expulsion of matter in the form of highly supersonic outflows. Although this phenomenon has been s…

astro-ph2005★ 75 cited

Spatially resolved PAH emission in the inner disks of Herbig Ae/Be stars

Emilie Habart, Antonella Natta, Leonardo Testi +1

We present adaptive optics high angular resolution ($\sim0.1\arcsec$) spectroscopic observations in the 3 \um region of eight well known Herbig Ae/Be stars with circumstellar disks…

astro-ph2005★ 250 cited

The Origin of Massive O-type Field Stars. Part II: Field O stars as runaways

W. J. de Wit, L. Testi, F. Palla +1

In two papers we try to confirm that all Galactic high-mass stars are formed in a cluster environment, by excluding that O-type stars found in the Galactic field actually formed th…

astro-ph2005★ 139 cited

A detailed study of the rotating toroids in G31.41+0.31 and G24.78+0.08

Maria T. Beltran, Riccardo Cesaroni, Roberto Neri +4

We present the results of high angular resolution millimeter observations of gas and dust toward G31.41+0.31 and G24.78+0.08, two high-mass star forming regions where four rotating…

astro-ph2005★ 22 cited

Relative Evolutionary Time Scale of Hot Molecular Cores with Respect to Ultra Compact HII Regions

R. S. Furuya, R. Cesaroni, S. Takahashi +4

Using the Owens Valley and Nobeyama Radio Observatory interferometers, we carried out an unbiased search for hot molecular cores and ultracompact UC HII regions toward the high-mas…