Search Publications

Distance determination for RAVE stars using stellar models. III. The nature of the RAVE survey and Milky Way chemistry
DOI: 10.1051/0004-6361/201116715 Bibcode: 2011A&A...532A.113B

Gilmore, G.; Freeman, K. C.; Munari, U. +19 more

We apply the method of Burnett & Binney (2010, MNRAS, 407, 339) for the determination of stellar distances and parameters to the internal catalogue of the RAdial Velocity Experiment (RAVE; Steinmetz et al. 2006, AJ, 132, 1645). Subsamples of stars that either have Hipparcos parallaxes or belong to well-studied clusters inspire confidence in th…

2011 Astronomy and Astrophysics
Hipparcos 54
Titan's obliquity as evidence of a subsurface ocean?
DOI: 10.1051/0004-6361/201116578 Bibcode: 2011A&A...530A.141B

Karatekin, Ö.; Baland, R. -M.; van Hoolst, T. +1 more

On the basis of gravity and radar observations with the Cassini spacecraft, the moment of inertia of Titan and the orientation of Titan's rotation axis have been estimated in recent studies. According to the observed orientation, Titan is close to the Cassini state. However, the observed obliquity is inconsistent with the estimate of the moment of…

2011 Astronomy and Astrophysics
Cassini 54
MHD wave transmission in the Sun's atmosphere
DOI: 10.1051/0004-6361/201117356 Bibcode: 2011A&A...534A..65S

Berrilli, F.; Del Moro, D.; Stangalini, M. +1 more

Magnetohydrodynamics (MHD) wave propagation inside the Sun's atmosphere is closely related to the magnetic field topology. For example, magnetic fields are able to lower the cutoff frequency for acoustic waves, thus allowing the propagation of waves that would otherwise be trapped below the photosphere into the upper atmosphere. In addition, MHD w…

2011 Astronomy and Astrophysics
Hinode 54
Ensemble X-ray variability of active galactic nuclei from serendipitous source catalogues
DOI: 10.1051/0004-6361/201118072 Bibcode: 2011A&A...536A..84V

Trevese, D.; Vagnetti, F.; Turriziani, S.

Context. The X-ray variability of the active galactic nuclei (AGN) has been most often investigated with studies of individual, nearby sources, and only a few ensemble analyses have been applied to large samples in wide ranges of luminosity and redshift.
Aims: We aim to determine the ensemble variability properties of two serendipitously sele…

2011 Astronomy and Astrophysics
XMM-Newton 53
New insight into the formation of hexamethylenetetramine (HMT) in interstellar and cometary ice analogs
DOI: 10.1051/0004-6361/201116688 Bibcode: 2011A&A...530A.128V

Vinogradoff, V.; Duvernay, F.; Danger, G. +2 more


Aims: We investigate the purely thermal formation of hexamethylenetetramine (HMT, C6H12N4) in interstellar ice analogs from non-photolysed ice and compare our results with those for the formation from photolysed ice.
Methods: We use Fourier transform-infrared spectroscopy to follow residue formation from …

2011 Astronomy and Astrophysics
Rosetta 53
The effect of environment on star forming galaxies at redshift. I. First insight from PACS
DOI: 10.1051/0004-6361/201015672 Bibcode: 2011A&A...532A.145P

Berta, S.; Magnelli, B.; Nordon, R. +33 more

We use deep 70, 100 and 160 µm observations taken with PACS, the Photodetector Array Camera and Spectrometer on board of Herschel, as part of the PACS Evolutionary Probe (PEP) guaranteed time, to study the relation between star formation rate and environment at redshift ~ 1 in the GOODS-S and GOODS-N fields. We use the SDSS spectroscopic cat…

2011 Astronomy and Astrophysics
Herschel 53
GOODS-Herschel: the impact of galaxy-galaxy interactions on the far-infrared properties of galaxies
DOI: 10.1051/0004-6361/201117476 Bibcode: 2011A&A...535A..60H

Magnelli, B.; Altieri, B.; Aussel, H. +15 more


Aims: We study the impact of galaxy-galaxy interactions on the far-infrared properties of galaxies and its evolution at 0 < z < 1.2.
Methods: Using the high-z galaxies in the fields of Great Observatories Origins Deep Survey (GOODS) observed by the Herschel Space Observatory in the framework of the GOODS-Herschel key program and th…

2011 Astronomy and Astrophysics
AKARI Herschel 52
Variable X-ray absorption in the mini-BAL QSO PG 1126-041
DOI: 10.1051/0004-6361/201117732 Bibcode: 2011A&A...536A..49G

Cappi, M.; Ponti, G.; Vignali, C. +7 more

Context. X-ray studies of active galactic nuclei (AGN) with powerful nuclear winds are important for constraining the physics of the inner accretion/ejection flow around supermassive black holes (SMBHs) and for understanding the impact of such winds on the AGN environment.
Aims: Our main scientific goal is to constrain the properties of the c…

2011 Astronomy and Astrophysics
XMM-Newton 52
The 22 May 2007 B-class flare: new insights from Hinode observations
DOI: 10.1051/0004-6361/201014906 Bibcode: 2011A&A...526A...1D

Mason, H. E.; Del Zanna, G.; Bradshaw, S. J. +2 more

We present multi-wavelength observations of a small B-class flare which occurred on the Sun on 2007 May 22. The observations include data from Hinode, GOES, TRACE and the Nobeyama Radioheliograph. We obtained spatially and spectrally-resolved information from the Hinode EUV Imaging Spectrometer (EIS) during this event. The temporal and temperature…

2011 Astronomy and Astrophysics
Hinode 51
An optical/NIR survey of globular clusters in early-type galaxies. II. Ages of globular cluster systems and the relation to galaxy morphology
DOI: 10.1051/0004-6361/201015683 Bibcode: 2011A&A...525A..20C

Larsen, S. S.; Kuntschner, H.; Anders, P. +5 more

Context. Some photometric studies of extragalactic globular cluster (GC) systems using the optical and near-infrared colour combination have suggested the presence of a large fraction of intermediate-age (2-8 Gyr) GCs.
Aims: We investigate the age distributions of GC systems in 14 E/S0 galaxies.
Methods: We carried out a differential com…

2011 Astronomy and Astrophysics
eHST 51