Search Publications

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
Two formation channels of ultra-compact dwarf galaxies in Hickson compact groups
DOI: 10.1051/0004-6361/201015353 Bibcode: 2011A&A...525A..86D

Mendes de Oliveira, C.; Hilker, M.; Ziegler, B. L. +3 more

Context. The formation of ultra-compact dwarf galaxies (UCDs) is believed to be driven by interaction, and UCDs are abundant in the cores of galaxy clusters, environments that mark the end-point of galaxy evolution. Nothing is known about the properties of UCDs in compact groups of galaxies, environments where most of galaxy evolution and interact…

2011 Astronomy and Astrophysics
eHST 50
Radial profiles of Fe abundance in the intracluster medium of nearby clusters observed with XMM-Newton
DOI: 10.1051/0004-6361/200913432 Bibcode: 2011A&A...527A.134M

Matsushita, K.


Aims: The abundances of Fe in the intracluster medium of nearby (z < 0.08) clusters were measured up to 0.3 ~ 0.5r180.
Methods: We analyzed 28 clusters of galaxies observed with XMM-Newton. We derived Fe abundances from the flux ratios of Fe lines to the continuum within an energy range of 3.5-6 keV to minimize and evaluate…

2011 Astronomy and Astrophysics
XMM-Newton 50
Image reconstruction in optical interferometry: benchmarking the regularization
DOI: 10.1051/0004-6361/201016263 Bibcode: 2011A&A...533A..64R

Thiébaut, E.; Malbet, F.; Renard, S.

Context. With the advent of visible and infrared long-baseline interferometers with more than two telescopes, both the size and the completeness of interferometric data sets have significantly increased, allowing images based on models with no a priori assumptions to be reconstructed with an aperture synthesis technique.
Aims: Our main object…

2011 Astronomy and Astrophysics
eHST 50
GRB 091127/SN 2009nz and the VLT/X-shooter spectroscopy of its host galaxy: probing the faint end of the mass-metallicity relation
DOI: 10.1051/0004-6361/201117726 Bibcode: 2011A&A...535A.127V

Covino, S.; D'Avanzo, P.; Sánchez-Ramírez, R. +36 more

We perform a detailed study of the gamma-ray burst GRB 091127/SN 2009nz host galaxy at z = 0.490 using the VLT/X-shooter spectrograph in slit and integral-field unit (IFU) mode. From the analysis of the optical and X-ray afterglow data obtained from ground-based telescopes and Swift-XRT, we confirm the presence of a bump associated with SN 2009nz …

2011 Astronomy and Astrophysics
eHST 49