Search Publications

Molecular line emission in NGC 1068 imaged with ALMA. I. An AGN-driven outflow in the dense molecular gas
DOI: 10.1051/0004-6361/201423843 Bibcode: 2014A&A...567A.125G

Tacconi, L. J.; Hunt, L. K.; Colina, L. +23 more


Aims: We investigate the fueling and the feedback of star formation and nuclear activity in NGC 1068, a nearby (D = 14 Mpc) Seyfert 2 barred galaxy, by analyzing the distribution and kinematics of the molecular gas in the disk. We aim to understand if and how gas accretion can self-regulate.
Methods: We have used the A…

2014 Astronomy and Astrophysics
eHST 395
The frequency of planetary debris around young white dwarfs
DOI: 10.1051/0004-6361/201423691 Bibcode: 2014A&A...566A..34K

Gänsicke, B. T.; Koester, D.; Farihi, J.

Context. Heavy metals in the atmospheres of white dwarfs are thought in many cases to be accreted from a circumstellar debris disk, which was formed by the tidal disruption of a rocky planetary body within the Roche radius of the star. The abundance analysis of photospheric elements and conclusions about the chemical composition of the accreted ma…

2014 Astronomy and Astrophysics
eHST 383
The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types
DOI: 10.1051/0004-6361/201322489 Bibcode: 2014A&A...568A..62D

Lebouteiller, Vianney; De Looze, Ilse; Baes, Maarten +19 more


Aims: We analyze the applicability of far-infrared fine-structure lines [Cii] 158 µm, [Oi] 63 µm, and [Oiii] 88 µm to reliably trace the star formation rate (SFR) in a sample of low-metallicity dwarf galaxies from the Herschel Dwarf Galaxy Survey and, furthermore, extend the analysis to a broad sample of galaxies of various …

2014 Astronomy and Astrophysics
Herschel ISO 370
Planck 2013 results. XXV. Searches for cosmic strings and other topological defects
DOI: 10.1051/0004-6361/201321621 Bibcode: 2014A&A...571A..25P

Miville-Deschênes, M. -A.; Bernard, J. -P.; Planck Collaboration +225 more

Planck data have been used to provide stringent new constraints on cosmic strings and other defects. We describe forecasts of the CMB power spectrum induced by cosmic strings, calculating these from network models and simulations using line-of-sight Boltzmann solvers. We have studied Nambu-Goto cosmic strings, as well as field theory strings for w…

2014 Astronomy and Astrophysics
Planck 352
Planck 2013 results. XII. Diffuse component separation
DOI: 10.1051/0004-6361/201321580 Bibcode: 2014A&A...571A..12P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +258 more

Planck has produced detailed all-sky observations over nine frequency bands between 30 and 857 GHz. These observations allow robust reconstruction of the primordial cosmic microwave background (CMB) temperature fluctuations over nearly the full sky, as well as new constraints on Galactic foregrounds, including thermal dust and line emission from m…

2014 Astronomy and Astrophysics
Planck 290
Gaia FGK benchmark stars: Metallicity
DOI: 10.1051/0004-6361/201322440 Bibcode: 2014A&A...564A.133J

Montes, D.; de Laverny, P.; Cantat-Gaudin, T. +22 more

Context. To calibrate automatic pipelines that determine atmospheric parameters of stars, one needs a sample of stars, or "benchmark stars", with well-defined parameters to be used as a reference.
Aims: We provide detailed documentation of the iron abundance determination of the 34 FGK-type benchmark stars that are selected to be the pillars …

2014 Astronomy and Astrophysics
Gaia 273
Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation
DOI: 10.1051/0004-6361/201322093 Bibcode: 2014A&A...571A..30P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +239 more

We present new measurements of cosmic infrared background (CIB) anisotropies using Planck. Combining HFI data with IRAS, the angular auto- and cross-frequency power spectrum is measured from 143 to 3000 GHz, and the auto-bispectrum from 217 to 545 GHz. The total areas used to compute the CIB power spectrum and bispectrum are about 2240 and 4400 de…

2014 Astronomy and Astrophysics
Herschel Planck 260
The evolution of the dust and gas content in galaxies
DOI: 10.1051/0004-6361/201322835 Bibcode: 2014A&A...562A..30S

Berta, S.; Magnelli, B.; Nordon, R. +36 more

We use deep Herschel observations taken with both PACS and SPIRE imaging cameras to estimate the dust mass of a sample of galaxies extracted from the GOODS-S, GOODS-N and the COSMOS fields. We divide the redshift-stellar mass (Mstar)-star formation rate (SFR) parameter space into small bins and investigate average properties over this g…

2014 Astronomy and Astrophysics
Herschel 247
Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove
DOI: 10.1051/0004-6361/201321556 Bibcode: 2014A&A...571A..27P

Bernard, J. -P.; Planck Collaboration; Aghanim, N. +181 more

Our velocity relative to the rest frame of the cosmic microwave background (CMB) generates a dipole temperature anisotropy on the sky which has been well measured for more than 30 years, and has an accepted amplitude of v/c = 1.23 × 10-3, or v = 369. In addition to this signal generated by Doppler boosting of the CMB monopole, our motio…

2014 Astronomy and Astrophysics
Planck 244
The Sloan Digital Sky Survey quasar catalog: tenth data release
DOI: 10.1051/0004-6361/201322691 Bibcode: 2014A&A...563A..54P

Finley, Hayley; Pâris, Isabelle; Petitjean, Patrick +47 more

We present the Data Release 10 Quasar (DR10Q) catalog from the Baryon Oscillation Spectroscopic Survey (BOSS) of the Sloan Digital Sky Survey III. The catalog includes all BOSS objects that were targeted as quasar candidates during the first 2.5 years of the survey and that are confirmed as quasars via visual inspection of the spectra, have lumino…

2014 Astronomy and Astrophysics
XMM-Newton 234