806 citations · 2.5k across the 15 of their papers we have counts for
15 papers
The ATLASGAL survey: distribution of cold dust in the Galactic plane. Combination with Planck data
T. Csengeri, A. Weiss, F. Wyrowski +9
Sensitive ground-based submillimeter surveys, such as ATLASGAL, provide a global view on the distribution of cold dense gas in the Galactic plane. Here we use the 353 GHz maps from…
Detection of two power-law tails in the probability distribution functions of massive GMCs
N. Schneider, S. Bontemps, P. Girichidis +20
We report the novel detection of complex high-column density tails in the probability distribution functions (PDFs) for three high-mass star-forming regions (CepOB3, MonR2, NGC6334…
SiO emission from low- and high-velocity shocks in Cygnus-X massive dense clumps
A. Duarte-Cabral, S. Bontemps, F. Motte +4
We used PdBI observations of SiO (2-1) to investigate the morphology and profile of the SiO emission within several massive dense clumps (MDCs) in Cygnus-X. We find that most molec…
Understanding star formation in molecular clouds II. Signatures of gravitational collapse of IRDCs
N. Schneider, T. Csengeri, R. S. Klessen +6
We analyse column density and temperature maps derived from Herschel dust continuum observations of a sample of massive infrared dark clouds (G11.11-0.12, G18.82-0.28, G28.37+0.07,…
The Dependence of Protostellar Luminosity on Environment in the Cygnus-X Star-Forming Complex
E. Kryukova, S. T. Megeath, J. L. Hora +7
The Cygnus-X star-forming complex is one of the most active regions of low and high mass star formation within 2 kpc of the Sun. Using mid-infrared photometry from the IRAC and MIP…
Characterizing the structure of diffuse emission in Hi-GAL maps
D. Elia, F. Strafella, N. Schneider +18
We present a study of the structure of the Galactic interstellar medium through the Delta-variance technique, related to the power spectrum and the fractal properties of infrared/s…
CO outflows from high-mass Class 0 protostars in Cygnus-X
A. Duarte-Cabral, S. Bontemps, F. Motte +3
As natural consequences of the accretion process, outflows are one of the few (indirect) tracers of accretion. We used CO(2-1) PdBI observations towards 6 MDCs in Cygnus-X, contain…
Young stellar clusters in the Rosette molecular cloud. Arguments against triggered star formation
L. Cambrésy, G. Marton, O. Feher +2
The Rosette complex is a well studied region of the galactic plane which presents the apparent characteristics of a triggered star forming region. This is however still debated as…
The first Hi-GAL observations of the outer Galaxy: a look to star formation in the third Galactic quadrant in the longitude range 216.5 < l < 225.5
D. Elia, S. Molinari, Y. Fukui +17
We present the first Herschel PACS and SPIRE photometric observations in a portion of the outer Galaxy ( and $-2^{\circ} \lesssi…
Discovery of an extremely bright submillimeter galaxy at z=3.93
J. -F. Lestrade, F. Combes, P. Salome +4
Serendipitously we have discovered a rare, bright submillimeter galaxy (SMG) with a flux density of 30 +/- 2 mJy at lambda=1.2mm, using MAMBO2 at the IRAM 30-meter millimeter teles…
Gas dynamics in Massive Dense Cores in Cygnus-X
T. Csengeri, S. Bontemps, N. Schneider +2
We study the kinematic properties of dense gas surrounding massive protostars recognized by Bontemps et a. (2010) in a sample of five Massive Dense Cores in Cygnus-X. We investigat…
Clouds, filaments and protostars: the Herschel Hi-GAL Milky Way
S. Molinari, B. Swinyard, J. Bally +121
We present the first results from the science demonstration phase for the Hi-GAL survey, the Herschel key-project that will map the inner Galactic Plane of the Milky Way in 5 bands…
The Herschel first look at protostars in the Aquila Rift
S. Bontemps, Ph. Andre, V. Konyves +40
As part of the science demonstration phase of the Herschel mission of the Gould Belt Key Program, the Aquila Rift molecular complex has been observed. The complete ~ 3.3deg x 3.3de…
Dynamic star formation in the massive DR21 filament
N. Schneider, T. Csengeri, S. Bontemps +5
The formation of massive stars is a highly complex process in which it is not clear whether the star-forming gas is in global gravitational collapse or in an equilibrium state, sup…
The earliest phases of high-mass star formation: a 3 square degree millimeter continuum mapping of Cygnus X
Frédérique Motte, S. Bontemps, P. Schilke +3
We have made an extensive 1.2mm continuum mosaicing study of the Cygnus X molecular cloud complex using the MAMBO cameras at the IRAM 30 m telescope. We then compared our mm maps w…