Search Publications

OSIRIS observations of meter-sized exposures of H2O ice at the surface of 67P/Churyumov-Gerasimenko and interpretation using laboratory experiments
DOI: 10.1051/0004-6361/201525977 Bibcode: 2015A&A...583A..25P

Jorda, L.; Lamy, P. L.; Bertaux, J. -L. +52 more

Since OSIRIS started acquiring high-resolution observations of the surface of the nucleus of comet 67P/Churyumov-Gerasimenko, over one hundred meter-sized bright spots have been identified in numerous types of geomorphologic regions, but mostly located in areas receiving low insolation. The bright spots are either clustered, in debris fields close…

2015 Astronomy and Astrophysics
Rosetta 100
Photometric properties of comet 67P/Churyumov-Gerasimenko from VIRTIS-M onboard Rosetta
DOI: 10.1051/0004-6361/201526307 Bibcode: 2015A&A...583A..31C

Bellucci, G.; Mottola, S.; Fornasier, S. +17 more


Aims: We investigate the nucleus photometric properties of the comet 67P/Churyumov-Gerasimenko as observed by the Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) onboard the Rosetta spacecraft. Both full-disk and disk-resolved images of the comet have been analyzed, deriving light and phase curves as well as a photometric reduction…

2015 Astronomy and Astrophysics
Rosetta 98
Planck 2013 results. XXXII. The updated Planck catalogue of Sunyaev-Zeldovich sources
DOI: 10.1051/0004-6361/201525787 Bibcode: 2015A&A...581A..14P

Böhringer, H.; Kneissl, R.; Dahle, H. +275 more

We update the all-sky Planck catalogue of 1227 clusters and cluster candidates (PSZ1) published in March 2013, derived from detections of the Sunyaev-Zeldovich (SZ) effect using the first 15.5 months of Planck satellite observations. As an addendum, we deliver an updated version of the PSZ1 catalogue, reporting the further confirmation of 86 Planc…

2015 Astronomy and Astrophysics
Planck 97
Occurrence of radio halos in galaxy clusters. Insight from a mass-selected sample
DOI: 10.1051/0004-6361/201526420 Bibcode: 2015A&A...580A..97C

Brunetti, G.; Kale, R.; Venturi, T. +4 more

Context. Giant radio halos (RH) are diffuse Mpc-scale synchrotron sources detected in some massive and merging galaxy clusters. An unbiased study of the statistical properties of RHs is crucial to constraining their origin and evolution.
Aims: We investigate the occurrence of RHs and its dependence on the cluster mass in a Sunyaev-Zel'dovich …

2015 Astronomy and Astrophysics
Planck XMM-Newton 96
Galaxy-wide outflows in z ~ 1.5 luminous obscured quasars revealed through near-IR slit-resolved spectroscopy
DOI: 10.1051/0004-6361/201425035 Bibcode: 2015A&A...574A..82P

Maiolino, R.; Salvato, M.; Marconi, A. +10 more


Aims: The co-evolution of galaxies and supermassive black holes (SMBHs) requires that some sort of feedback mechanism is operating during the active galactic nuclei (AGN) phases. AGN driven winds are the most likely candidates for such feedback mechanism, but direct observational evidence of their existence and of their effects on the host ga…

2015 Astronomy and Astrophysics
XMM-Newton eHST 96
Molecular depletion times and the CO-to-H2 conversion factor in metal-poor galaxies
DOI: 10.1051/0004-6361/201526553 Bibcode: 2015A&A...583A.114H

Maiolino, R.; Menten, K. M.; Hunt, L. K. +8 more

Tracing molecular hydrogen content with carbon monoxide in low-metallicity galaxies has been exceedingly difficult. Here we present a new effort, with IRAM 30-m observations of 12CO(1-0) of a sample of 8 dwarf galaxies having oxygen abundances ranging from 12 + log(O/H) ~ 7.7 to 8.4. CO emission is detected in all galaxies, including th…

2015 Astronomy and Astrophysics
eHST 96
Molecular gas content in strongly lensed z ~ 1.5-3 star-forming galaxies with low infrared luminosities
DOI: 10.1051/0004-6361/201424661 Bibcode: 2015A&A...577A..50D

Kneib, J. -P.; Schaerer, D.; Dessauges-Zavadsky, M. +10 more

To extend the molecular gas measurements to more typical star-forming galaxies (SFGs) with star formation rates SFR< 40 M yr-1 and stellar masses M< 2.5 × 1010M at z ~ 1.5-3, we have observed CO emission with the IRAM Plateau de Bure Interferometer and the IRAM 30 m telescope for five…

2015 Astronomy and Astrophysics
Herschel 92
Planck intermediate results. XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible
DOI: 10.1051/0004-6361/201424087 Bibcode: 2015A&A...576A.106P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +193 more

The Planck survey provides unprecedented full-sky coverage of the submillimetre polarized emission from Galactic dust. In addition to the information on the direction of the Galactic magnetic field, this also brings new constraints on the properties of dust. The dust grains that emit the radiation seen by Planck in the submillimetre also extinguis…

2015 Astronomy and Astrophysics
Planck 91
The VLT/NaCo large program to probe the occurrence of exoplanets and brown dwarfs in wide orbits. I. Sample definition and characterization
DOI: 10.1051/0004-6361/201323168 Bibcode: 2015A&A...573A.126D

Moutou, C.; Henning, T.; Alcalá, J. M. +28 more

Context. Young, close stars are ideal targets for searching planets using the direct imaging technique. The determination of stellar parameters is crucial for the interpretation of imaging survey results, particularly since the luminosity of substellar objects has a strong dependence on system age.
Aims: We have conducted a large program with…

2015 Astronomy and Astrophysics
XMM-Newton 91
What drives the dust activity of comet 67P/Churyumov-Gerasimenko?
DOI: 10.1051/0004-6361/201525828 Bibcode: 2015A&A...583A..12G

Blum, J.; Gundlach, B.; Keller, H. U. +1 more

Context. The gas-driven dust activity of comets is still an unsolved question in cometary physics. Homogeneous dust layers composed of micrometer-sized grains possess tensile strengths of ~1 kPa, which is far higher than typical gas pressures caused by the sublimation of the ices beneath the covering dust layer. This implies that the dust grains c…

2015 Astronomy and Astrophysics
Rosetta 89