Search Publications

Far-infrared study of tracers of oxygen chemistry in diffuse clouds
DOI: 10.1051/0004-6361/201526473 Bibcode: 2016A&A...585A..76W

Menten, K. M.; Neufeld, D. A.; Stutzki, J. +8 more

Context. The chemistry of the diffuse interstellar medium rests upon three pillars: exothermic ion-neutral reactions ("cold chemistry"), endothermic neutral-neutral reactions with significant activation barriers ("warm chemistry"), and reactions on the surfaces of dust grains. While warm chemistry becomes important in the shocks associated with tu…

2016 Astronomy and Astrophysics
Herschel 34
First simultaneous SST/CRISP and IRIS observations of a small-scale quiet Sun vortex
DOI: 10.1051/0004-6361/201527440 Bibcode: 2016A&A...586A..25P

Doyle, J. G.; Scullion, E.; Tziotziou, K. +3 more

Context. Ubiquitous small-scale vortices have recently been found in the lower atmosphere of the quiet Sun in state-of-the-art solar observations and in numerical simulations.
Aims: We investigate the characteristics and temporal evolution of a granular-scale vortex and its associated upflows through the photosphere and chromosphere of a quie…

2016 Astronomy and Astrophysics
IRIS 34
A mini outburst from the nightside of comet 67P/Churyumov-Gerasimenko observed by the OSIRIS camera on Rosetta
DOI: 10.1051/0004-6361/201527744 Bibcode: 2016A&A...596A..89K

Jorda, L.; Lara, L. M.; Lamy, P. +40 more

Context. On 12 March 2015 the OSIRIS WAC camera onboard the ESA Rosetta spacecraft orbiting comet 67P/Churyumov-Gerasimenko observed a small outburst originating from the Imhotep region at the foot of the big lobe of the comet. These measurements are unique since it was the first time that the initial phase of a transient outburst event could be d…

2016 Astronomy and Astrophysics
Rosetta 34
Probing the 2D temperature structure of protoplanetary disks with Herschel observations of high-J CO lines
DOI: 10.1051/0004-6361/201526948 Bibcode: 2016A&A...591A..95F

Fedele, D.; van Dishoeck, E. F.; Bruderer, S. +2 more

The gas temperature structure of protoplanetary disks is a key ingredient for interpreting various disk observations and for quantifying the subsequent evolution of these systems. The comparison of low- and mid-J CO rotational lines is a powerful tool for assessing the temperature gradient in the warm molecular layer of disks. Spectrally resolved …

2016 Astronomy and Astrophysics
Herschel 34
Planck intermediate results. XL. The Sunyaev-Zeldovich signal from the Virgo cluster
DOI: 10.1051/0004-6361/201527743 Bibcode: 2016A&A...596A.101P

Kneissl, R.; Miville-Deschênes, M. -A.; Bernard, J. -P. +202 more

The Virgo cluster is the largest Sunyaev-Zeldovich (SZ) source in the sky, both in terms of angular size and total integrated flux. Planck's wide angular scale and frequency coverage, together with its high sensitivity, enable a detailed study of this big object through the SZ effect. Virgo is well resolved by Planck, showing an elongated structur…

2016 Astronomy and Astrophysics
Planck XMM-Newton 34
A model of short-lived outbursts on the 67P from fractured terrains
DOI: 10.1051/0004-6361/201628365 Bibcode: 2016A&A...593A..76S

Keller, H. U.; Hartogh, P.; Rezac, L. +2 more


Aims: We develop a physical model to explain the potent outbursts that occurred in the fractured terrain of comet 67P near perihelion, and predict its temporal characteristics.
Methods: The feasibility of the proposed mechanism is studied using a numerical model accounting for the relevant microscopic/macroscopic processes. We rely on th…

2016 Astronomy and Astrophysics
Rosetta 33
Multi-wavelength characterisation of z ~ 2 clustered, dusty star-forming galaxies discovered by Planck
DOI: 10.1051/0004-6361/201425226 Bibcode: 2016A&A...585A..54F

Le Floc'h, E.; Dole, H.; Lagache, G. +9 more

We report the discovery of PHz G95.5-61.6, a complex structure detected in emission in the Planck all-sky survey that corresponds to two over-densities of high-redshift (I.e. z> 1) galaxies. This is the first source from the Planck catalogue of high-z candidates (proto-clusters and lensed systems) that has been completely characterised with fol…

2016 Astronomy and Astrophysics
Herschel Planck 33
Cosmic microwave background reconstruction from WMAP and Planck PR2 data
DOI: 10.1051/0004-6361/201527822 Bibcode: 2016A&A...591A..50B

Starck, J. -L.; Sureau, F.; Bobin, J.

We describe a new estimate of the cosmic microwave background (CMB) intensity map reconstructed by a joint analysis of the full Planck 2015 data (PR2) and nine years of WMAP data. The proposed map provides more than a mere update of the CMB map introduced in a previous paper since it benefits from an improvement of the component separation method …

2016 Astronomy and Astrophysics
Planck 33
Galactic cold cores. VII. Filament formation and evolution: Methods and observational constraints
DOI: 10.1051/0004-6361/201526263 Bibcode: 2016A&A...591A..90R

Bernard, J. -P.; Juvela, M.; Marshall, D. J. +15 more

Context. The association of filaments with protostellar objects has made these structures a priority target in star formation studies. However, little is known about the link between filament properties and their local environment.
Aims: The datasets from the Herschel Galactic Cold cores key programme allow for a statistical study of filament…

2016 Astronomy and Astrophysics
Herschel 33
Star-forming dwarf galaxies in the Virgo cluster: the link between molecular gas, atomic gas, and dust
DOI: 10.1051/0004-6361/201628123 Bibcode: 2016A&A...590A..27G

Riguccini, L.; De Looze, I.; Hunt, L. K. +11 more

We present 12CO(1-0) and 12CO(2-1) observations of a sample of 20 star-forming dwarfs selected from the Herschel Virgo Cluster Survey, with oxygen abundances ranging from 12 + log (O / H) ~ 8.1 to 8.8. CO emission is observed in ten galaxies and marginally detected in another one. CO fluxes correlate with the FIR 250 µm…

2016 Astronomy and Astrophysics
Herschel 33