Search Publications

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
On the relationship of shock waves to flares and coronal mass ejections
DOI: 10.1051/0004-6361/201116799 Bibcode: 2011A&A...531A..31N

Hillaris, A.; Preka-Papadema, P.; Nindos, A. +1 more

Context. Metric type II bursts are the most direct diagnostic of shock waves in the solar corona.
Aims: There are two main competing views about the origin of coronal shocks: that they originate in either blast waves ignited by the pressure pulse of a flare or piston-driven shocks due to coronal mass ejections (CMEs). We studied three well-ob…

2011 Astronomy and Astrophysics
SOHO 51
VLT-VIMOS integral field spectroscopy of luminous and ultraluminous infrared galaxies. III. The atlas of the stellar and ionized gas distribution
DOI: 10.1051/0004-6361/201014879 Bibcode: 2011A&A...527A..60R

Colina, L.; Monreal-Ibero, A.; Arribas, S. +3 more

Context. Luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) are much more numerous at higher redshifts than locally, dominating the star-formation rate density at redshifts ~1-2. Therefore, they are important objects in order to understand how galaxies form and evolve through cosmic time. Local samples provide a unique opportunity to …

2011 Astronomy and Astrophysics
eHST 51
The hard X-ray emission of Centaurus A
DOI: 10.1051/0004-6361/201016020 Bibcode: 2011A&A...531A..70B

Terrier, R.; Jean, P.; Beckmann, V. +2 more

Context. The radio galaxy Cen A has been detected all the way up to the TeV energy range. This raises the question about the dominant emission mechanisms in the high-energy domain.
Aims: Spectral analysis allows us to put constraints on the possible emission processes. Here we study the hard X-ray emission, in order to distinguish between a t…

2011 Astronomy and Astrophysics
INTEGRAL 51
Witnessing the magnetospheric boundary at work in Vela X-1
DOI: 10.1051/0004-6361/201116482 Bibcode: 2011A&A...529A..52D

Santangelo, A.; Doroshenko, V.; Suleimanov, V.

We present an analysis of the Vela X-1 "off-states" based on Suzaku observations taken in June 2008. Defined as states in which the flux suddenly decreases below the instrumental sensitivity, these "off-states" have been interpreted by several authors as the onset of the "propeller regime". For the first time ever, however, we find that the source…

2011 Astronomy and Astrophysics
Suzaku 51
Asymmetries of the Stokes V profiles observed by HINODE SOT/SP in the quiet Sun
DOI: 10.1051/0004-6361/201016096 Bibcode: 2011A&A...530A..14V

Sánchez Almeida, J.; Viticchié, B.


Aims: A recent analysis of polarization measurements of HINODE SOT/SP in the quiet Sun pointed out very complex shapes of Stokes V profiles. Here we present the first classification of the SOT/SP circular polarization measurements with the aim of highlighting exhaustively the whole variety of Stokes V shapes emerging from the quiet Sun.

2011 Astronomy and Astrophysics
Hinode 51
A new comprehensive 2D model of the point spread functions of the XMM-Newton EPIC telescopes: spurious source suppression and improved positional accuracy
DOI: 10.1051/0004-6361/201117525 Bibcode: 2011A&A...534A..34R

Read, A. M.; Saxton, R. D.; Rosen, S. R. +1 more


Aims: We describe here a new full 2D parameterization of the PSFs of the three XMM-Newton EPIC telescopes as a function of instrument, energy, off-axis angle and azimuthal angle, covering the whole field-of-view (FoV) of the three EPIC detectors. It models the general PSF envelopes, the primary and secondary spokes, their radial dependencies,…

2011 Astronomy and Astrophysics
XMM-Newton 51