Search Publications

A study of deuterated water in the low-mass protostar IRAS 16293-2422
DOI: 10.1051/0004-6361/201117627 Bibcode: 2012A&A...539A.132C

Ceccarelli, C.; Caux, E.; Vastel, C. +6 more

Context. Water is a primordial species in the emergence of life, and comets may have brought a large fraction to Earth to form the oceans. To understand the evolution of water from the first stages of star formation to the formation of planets and comets, the HDO/H2O ratio is a powerful diagnostic.
Aims: Our aim is to determine pre…

2012 Astronomy and Astrophysics
Herschel 118
The circumstellar disk of AB Aurigae: evidence for envelope accretion at late stages of star formation?
DOI: 10.1051/0004-6361/201219414 Bibcode: 2012A&A...547A..84T

Guilloteau, S.; Dutrey, A.; Piétu, V. +3 more


Aims: The circumstellar disk of AB Aurigae has garnered strong attention owing to the apparent existence of spirals at a relatively young stage and also the asymmetric disk traced in thermal dust emission. However, the physical conditions of the spirals are still not well understood. The origin of the asymmetric thermal emission is unclear. <…

2012 Astronomy and Astrophysics
eHST 116
Evaporating very small grains as tracers of the UV radiation field in photo-dissociation regions
DOI: 10.1051/0004-6361/201015915 Bibcode: 2012A&A...542A..69P

Joblin, C.; Pilleri, P.; Montillaud, J. +1 more

Context. In photo-dissociation regions (PDRs), polycyclic aromatic hydrocarbons (PAHs) may be produced by evaporation of very small grains (VSGs) by the impinging UV radiation field from a nearby star.
Aims: We quantitatively investigate the transition zone between evaporating VSGs (eVSGs) and PAHs in several PDRs.
Methods: We studied th…

2012 Astronomy and Astrophysics
ISO 114
The Earliest Phases of Star Formation (EPoS): a Herschel key program. The precursors to high-mass stars and clusters
DOI: 10.1051/0004-6361/201219232 Bibcode: 2012A&A...547A..49R

Henning, Th.; Krause, O.; Balog, Z. +14 more

Context. Stars are born deeply embedded in molecular clouds. In the earliest embedded phases, protostars emit the bulk of their radiation in the far-infrared wavelength range, where Herschel is perfectly suited to probe at high angular resolution and dynamic range. In the high-mass regime, the birthplaces of protostars are thought to be in the hig…

2012 Astronomy and Astrophysics
Herschel 113
Herschel measurements of the D/H and 16O/18O ratios in water in the Oort-cloud comet C/2009 P1 (Garradd)
DOI: 10.1051/0004-6361/201219744 Bibcode: 2012A&A...544L..15B

Küppers, M.; Hartogh, P.; Lellouch, E. +19 more

The D/H ratio in cometary water is believed to be an important indicator of the conditions under which icy planetesimals formed and can provide clues to the contribution of comets to the delivery of water and other volatiles to Earth. Available measurements suggest that there is isotopic diversity in the comet population. The Herschel Space Observ…

2012 Astronomy and Astrophysics
Herschel 108
Gravito-inertial and pressure modes detected in the B3 IV CoRoT target HD 43317
DOI: 10.1051/0004-6361/201218809 Bibcode: 2012A&A...542A..55P

Auvergne, M.; Baudin, F.; Poretti, E. +14 more

Context. OB stars are important building blocks of the Universe, but we have only a limited sample of them well understood enough from an asteroseismological point of view to provide feedback on the current evolutionary models. Our study adds one special case to this sample, with more observational constraints than for most of these stars.
Ai…

2012 Astronomy and Astrophysics
CoRoT 107
Modelling Herschel observations of hot molecular gas emission from embedded low-mass protostars
DOI: 10.1051/0004-6361/201117109 Bibcode: 2012A&A...537A..55V

Wolfire, M. G.; van Dishoeck, E. F.; Bruderer, S. +6 more


Aims: Young stars interact vigorously with their surroundings, as evident from the highly rotationally excited CO (up to Eu/k = 4000 K) and H2O emission (up to 600 K) detected by the Herschel Space Observatory in embedded low-mass protostars. Our aim is to construct a model that reproduces the observations quantitatively…

2012 Astronomy and Astrophysics
Herschel 107
Herschel images of Fomalhaut. An extrasolar Kuiper belt at the height of its dynamical activity
DOI: 10.1051/0004-6361/201118581 Bibcode: 2012A&A...540A.125A

Ivison, R. J.; Fridlund, M.; Blommaert, J. A. D. L. +33 more

Context. Fomalhaut is a young (2 ± 1 × 108 years), nearby (7.7 pc), 2 M star that is suspected to harbor an infant planetary system, interspersed with one or more belts of dusty debris.
Aims: We present far-infrared images obtained with the Herschel Space Observatory with an angular resolution between 5.7'' and 36.7'' a…

2012 Astronomy and Astrophysics
AKARI Herschel 106
Spatially coupled inversion of spectro-polarimetric image data. I. Method and first results
DOI: 10.1051/0004-6361/201220220 Bibcode: 2012A&A...548A...5V

van Noort, M.

Context. When inverting solar spectra, image degradation effects that are present in the data are usually approximated or not considered.
Aims: We develop a data reduction method that takes these issues into account and minimizes the resulting errors.
Methods: By accounting for the diffraction PSF of the telescope during the inversions, …

2012 Astronomy and Astrophysics
Hinode 105
An icy Kuiper belt around the young solar-type star HD 181327
DOI: 10.1051/0004-6361/201117714 Bibcode: 2012A&A...539A..17L

Pinte, C.; Ménard, F.; Duchêne, G. +18 more

Context. HD 181327 is a young main sequence F5/F6 V star belonging to the β Pictoris moving group (age ~12 Myr). It harbors an optically thin belt of circumstellar material at radius ~90 AU, presumed to result from collisions in a population of unseen planetesimals.
Aims: We aim to study the dust properties in the belt in d…

2012 Astronomy and Astrophysics
Herschel eHST 102