Search Publications

The solar type protostar IRAS16293-2422: new constraints on the physical structure
DOI: 10.1051/0004-6361/200913112 Bibcode: 2010A&A...519A..65C

Maret, S.; Ceccarelli, C.; Lis, D. C. +5 more

Context. The low mass protostar IRAS16293-2422 is a prototype Class 0 source in studies of the chemical structure during the initial phases of life of solar type stars.
Aims: To derive the chemical structure accurately, a precise determination of the source physical structure is required. The goal of this study is to derive the structure of I…

2010 Astronomy and Astrophysics
ISO 73
Water in low-mass star-forming regions with Herschel . HIFI spectroscopy of NGC 1333
DOI: 10.1051/0004-6361/201015100 Bibcode: 2010A&A...521L..30K

de Graauw, Th.; Liseau, R.; Braine, J. +64 more

“Water In Star-forming regions with Herschel” (WISH) is a key programme dedicated to studying the role of water and related species during the star-formation process and constraining the physical and chemical properties of young stellar objects. The Heterodyne Instrument for the Far-Infrared (HIFI) on the Herschel Space Observatory observed three …

2010 Astronomy and Astrophysics
Herschel 73
Near-IR integral field spectroscopy of ionizing stars and young stellar objects on the borders of H II regions
DOI: 10.1051/0004-6361/200913158 Bibcode: 2010A&A...510A..32M

Martins, F.; Zavagno, A.; Bouret, J. C. +2 more


Aims: We study three Galactic H ii regions - RCW 79, RCW 82, and RCW 120 - where triggered star formation is taking place. Two stellar populations are observed: the ionizing stars of each H ii region and young stellar objects on their borders. Our goal is to show that they represent two distinct populations, as expected from successive star-f…

2010 Astronomy and Astrophysics
AKARI 73
Spatial distribution of interstellar dust in the Sun's vicinity. Comparison with neutral sodium-bearing gas
DOI: 10.1051/0004-6361/200913962 Bibcode: 2010A&A...518A..31V

Lallement, R.; Vergely, J. -L.; Raimond, S. +1 more


Aims: 3D tomography of the interstellar dust and gas may be useful in many respects, from the physical and chemical evolution of the interstellar medium itself to foreground decontamination of the cosmic microwave background, or various studies of the environments of specific objects. However, while spectral data cubes of the galactic emissio…

2010 Astronomy and Astrophysics
Hipparcos 73
Superdense Massive Galaxies in the ESO Distant Cluster Survey (EDisCS)
DOI: 10.1088/2041-8205/721/1/L19 Bibcode: 2010ApJ...721L..19V

Fritz, J.; Moretti, A.; Vulcani, B. +9 more

We find a significant number of massive and compact galaxies in clusters from the ESO Distant Clusters Survey (EDisCS) at 0.4 < z < 1. They have similar stellar masses, ages, sizes, and axial ratios to local z ~ 0.04 compact galaxies in WIde field Nearby Galaxy clusters Survey (WINGS) clusters, and to z = 1.4-2 massive and passive galaxies f…

2010 The Astrophysical Journal
eHST 73
Radiolysis of ammonia-containing ices by energetic, heavy, and highly charged ions inside dense astrophysical environments
DOI: 10.1051/0004-6361/200912274 Bibcode: 2010A&A...509A..87P

Pilling, S.; Seperuelo Duarte, E.; da Silveira, E. F. +4 more

Deep inside dense molecular clouds and protostellar disks, interstellar ices are protected from stellar energetic UV photons. However, X-rays and energetic cosmic rays can penetrate inside these regions triggering chemical reactions, molecular dissociation, and evaporation processes. We present experimental studies of the interaction of heavy, hig…

2010 Astronomy and Astrophysics
ISO 73
Photospheric activity, rotation, and radial velocity variations of the planet-hosting star CoRoT-7
DOI: 10.1051/0004-6361/201014403 Bibcode: 2010A&A...520A..53L

Aigrain, S.; Alonso, R.; Auvergne, M. +11 more

Context. The CoRoT satellite has recently discovered the transits of an Earth-like planet across the disc of a late-type magnetically active star dubbed CoRoT-7, while a second planet was detected after filtering out the radial velocity (hereafter RV) variations due to stellar activity.
Aims: We investigate the magnetic activity of CoRoT-7 an…

2010 Astronomy and Astrophysics
CoRoT 73
Implications of a High Angular Resolution Image of the Sunyaev-Zel'Dovich Effect in RXJ1347-1145
DOI: 10.1088/0004-637X/716/1/739 Bibcode: 2010ApJ...716..739M

Ade, P.; Aguirre, J. E.; Devlin, M. J. +11 more

The most X-ray luminous cluster known, RXJ1347-1145 (z = 0.45), has been the object of extensive study across the electromagnetic spectrum. We have imaged the Sunyaev-Zel'dovich effect (SZE) at 90 GHz (λ = 3.3 mm) in RXJ1347-1145 at 10'' resolution with the 64 pixel MUSTANG bolometer array on the Green Bank Telescope, confirming a previously repor…

2010 The Astrophysical Journal
eHST 72
First results of the Herschel key program ``Dust, Ice and Gas In Time'' (DIGIT): Dust and gas spectroscopy of HD 100546
DOI: 10.1051/0004-6361/201014674 Bibcode: 2010A&A...518L.129S

Waters, L. B. F. M.; Maret, S.; Güdel, M. +40 more

Context. We present far-infrared spectroscopic observations, taken with the Photodetector Array Camera and Spectrometer (PACS) on the Herschel Space Observatory, of the protoplanetary disk around the pre-main-sequence star HD 100546. These observations are the first within the DIGIT Herschel key program, which aims to follow the evolution of dust,…

2010 Astronomy and Astrophysics
Herschel 72
Quiescent X-ray Emission From Cen X-4: A Variable Thermal Component
DOI: 10.1088/0004-637X/720/2/1325 Bibcode: 2010ApJ...720.1325C

Miller, Jon M.; Cackett, Edward M.; Wijnands, Rudy +1 more

The nearby neutron star low-mass X-ray binary, Cen X-4, has been in a quiescent state since its last outburst in 1979. Typically, quiescent emission from these objects consists of thermal emission (presumably from the neutron star surface) with an additional hard power-law tail of unknown nature. Variability has been observed during quiescence in …

2010 The Astrophysical Journal
Suzaku XMM-Newton 72