Search Publications

Anatomy of the AGN in NGC 5548. VI. Long-term variability of the warm absorber
DOI: 10.1051/0004-6361/201527808 Bibcode: 2016A&A...587A.129E

Kaastra, J. S.; Kriss, G. A.; Bianchi, S. +13 more

Context. We observed the archetypal Seyfert 1 galaxy NGC 5548 in 2013-2014 in the context of an extensive multiwavelength campaign involving several satellites, which revealed the source to be in an extraordinary state of persistent heavy obscuration.
Aims: We re-analyzed the archival grating spectra obtained by XMM-Newton and Chandra between…

2016 Astronomy and Astrophysics
XMM-Newton 35
The cause of spatial structure in solar He I 1083 nm multiplet images
DOI: 10.1051/0004-6361/201628490 Bibcode: 2016A&A...594A.104L

Joshi, Jayant; Carlsson, Mats; Leenaarts, Jorrit +2 more

Context. The He I 1083 nm is a powerful diagnostic for inferring properties of the upper solar chromosphere, in particular for the magnetic field. The basic formation of the line in one-dimensional models is well understood, but the influence of the complex three-dimensional structure of the chromosphere and corona has however never been investiga…

2016 Astronomy and Astrophysics
IRIS 35
A textbook example of ram-pressure stripping in the Hydra A/A780 cluster
DOI: 10.1051/0004-6361/201526641 Bibcode: 2016A&A...592A.154D

Rossetti, M.; Molendi, S.; De Grandi, S. +7 more

In the current epoch, one of the main mechanisms driving the growth of galaxy clusters is the continuous accretion of group-scale halos. In this process, the ram pressure applied by the hot intracluster medium on the gas content of the infalling group is responsible for stripping the gas from its dark-matter halo, which gradually leads to the viri…

2016 Astronomy and Astrophysics
Suzaku XMM-Newton 35
GK Persei and EX Hydrae: Intermediate polars with small magnetospheres
DOI: 10.1051/0004-6361/201628301 Bibcode: 2016A&A...591A..35S

Werner, K.; Ducci, L.; Doroshenko, V. +2 more

Observed hard X-ray spectra of intermediate polars are determined mainly by the accretion flow velocity at the white dwarf surface, which is normally close to the free-fall velocity. This allows us to estimate the white dwarf masses as the white dwarf mass-radius relation M - R and the expected free-fall velocities at the surface are well known. T…

2016 Astronomy and Astrophysics
INTEGRAL Suzaku 35
Electrical properties and porosity of the first meter of the nucleus of 67P/Churyumov-Gerasimenko. As constrained by the Permittivity Probe SESAME-PP/Philae/Rosetta
DOI: 10.1051/0004-6361/201628304 Bibcode: 2016A&A...591A..32L

Le Gall, Alice; Seidensticker, Klaus J.; Fischer, Hans-Herbert +7 more

Context. Comets are primitive objects, remnants of the volatile-rich planetesimals from which the solar system condensed. Knowing their structure and composition is thus crucial for the understanding of our origins. After the successful landing of Philae on the nucleus of 67P/Churyumov-Gerasimenko in November 2014, for the first time, the Rosetta …

2016 Astronomy and Astrophysics
Rosetta 35
Photospheric and coronal magnetic fields in six magnetographs. I. Consistent evolution of the bashful ballerina
DOI: 10.1051/0004-6361/201628096 Bibcode: 2016A&A...591A..78V

Mursula, Kalevi; Virtanen, Ilpo


Aims: We study the long-term evolution of photospheric and coronal magnetic fields and the heliospheric current sheet (HCS), especially its north-south asymmetry. Special attention is paid to the reliability of the six data sets used in this study and to the consistency of the results based on these data sets.
Methods: We use synoptic ma…

2016 Astronomy and Astrophysics
SOHO 34
Revealing the broad iron Kα line in Cygnus X-1 through simultaneous XMM-Newton, RXTE, and INTEGRAL observations
DOI: 10.1051/0004-6361/201424740 Bibcode: 2016A&A...589A..14D

Grinberg, Victoria; Pottschmidt, Katja; Staubert, Rüdiger +15 more

We report on the analysis of the broad Fe Kα line feature of Cyg X-1 in the spectra of four simultaneous hard intermediate state observations made with the X-ray Multiple Mirror mission (XMM-Newton), the Rossi X-ray Timing Explorer (RXTE), and the International Gamma-Ray Astrophysics Laboratory (INTEGRAL). The high quality of the XMM-Newton data t…

2016 Astronomy and Astrophysics
INTEGRAL XMM-Newton 34
Far-infrared study of tracers of oxygen chemistry in diffuse clouds
DOI: 10.1051/0004-6361/201526473 Bibcode: 2016A&A...585A..76W

Menten, K. M.; Neufeld, D. A.; Stutzki, J. +8 more

Context. The chemistry of the diffuse interstellar medium rests upon three pillars: exothermic ion-neutral reactions ("cold chemistry"), endothermic neutral-neutral reactions with significant activation barriers ("warm chemistry"), and reactions on the surfaces of dust grains. While warm chemistry becomes important in the shocks associated with tu…

2016 Astronomy and Astrophysics
Herschel 34
First simultaneous SST/CRISP and IRIS observations of a small-scale quiet Sun vortex
DOI: 10.1051/0004-6361/201527440 Bibcode: 2016A&A...586A..25P

Doyle, J. G.; Scullion, E.; Tziotziou, K. +3 more

Context. Ubiquitous small-scale vortices have recently been found in the lower atmosphere of the quiet Sun in state-of-the-art solar observations and in numerical simulations.
Aims: We investigate the characteristics and temporal evolution of a granular-scale vortex and its associated upflows through the photosphere and chromosphere of a quie…

2016 Astronomy and Astrophysics
IRIS 34
A mini outburst from the nightside of comet 67P/Churyumov-Gerasimenko observed by the OSIRIS camera on Rosetta
DOI: 10.1051/0004-6361/201527744 Bibcode: 2016A&A...596A..89K

Jorda, L.; Lara, L. M.; Lamy, P. +40 more

Context. On 12 March 2015 the OSIRIS WAC camera onboard the ESA Rosetta spacecraft orbiting comet 67P/Churyumov-Gerasimenko observed a small outburst originating from the Imhotep region at the foot of the big lobe of the comet. These measurements are unique since it was the first time that the initial phase of a transient outburst event could be d…

2016 Astronomy and Astrophysics
Rosetta 34