Search Publications

The accelerated build-up of the red sequence in high-redshift galaxy clusters
DOI: 10.1093/mnras/stw080 Bibcode: 2016MNRAS.457.2209C

Demarco, R.; Lidman, C.; Huertas-Company, M. +6 more

We analyse the evolution of the red sequence in a sample of galaxy clusters at redshifts 0.8 < z < 1.5 taken from the HAWK-I Cluster Survey (HCS). The comparison with the low-redshift (0.04 < z < 0.08) sample of the WIde-field Nearby Galaxy-cluster Survey (WINGS) and other literature results shows that the slope and intrinsic scatter o…

2016 Monthly Notices of the Royal Astronomical Society
eHST 35
Magnetically Dominated Parallel Interstellar Filaments in the Infrared Dark Cloud G14.225-0.506
DOI: 10.3847/0004-637X/832/2/186 Bibcode: 2016ApJ...832..186S

Zhang, Qizhou; Girart, Josep Miquel; Busquet, Gemma +2 more

The infrared dark cloud G14.225-0.506 (IRDC G14.2) displays a remarkable complex of parallel dense molecular filaments projected on the plane of the sky. Previous studies of dust emission and molecular lines have speculated whether magnetic fields could have played an important role in the formation of such elongated structures, which are hosts to…

2016 The Astrophysical Journal
Herschel 35
The Search for Extraterrestrial Intelligence in Earth's Solar Transit Zone
DOI: 10.1089/ast.2015.1358 Bibcode: 2016AsBio..16..259H

Heller, René; Pudritz, Ralph E.

Over the past few years, astronomers have detected thousands of planets and candidate planets by observing their periodic transits in front of their host stars. A related method, called transit spectroscopy, might soon allow studies of the chemical imprints of life in extrasolar planetary atmospheres. Here, we address the reciprocal question, name…

2016 Astrobiology
Hipparcos 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
Observation of an MHD Alfvén vortex in the slow solar wind
DOI: 10.1002/2015JA022248 Bibcode: 2016JGRA..121.3870R

Alexandrova, O.; Li, B.; Li, X. +1 more

In the solar wind, magnetic field power spectra usually show several power laws. In this paper, magnetic field data from the Cluster mission during an undisturbed interval of slow solar wind are analyzed at 0.28 Hz, near the spectral break point between the ion inertial and dissipation/dispersion ranges. Assuming Taylor's frozen-in condition, it c…

2016 Journal of Geophysical Research (Space Physics)
Cluster 35
Exploring the Venus global super-rotation using a comprehensive general circulation model
DOI: 10.1016/j.pss.2016.09.001 Bibcode: 2016P&SS..134....1M

Read, P. L.; Mendonça, J. M.

The atmospheric circulation in Venus is well known to exhibit strong super-rotation. However, the atmospheric mechanisms responsible for the formation of this super-rotation are still not fully understood. In this work, we developed a new Venus general circulation model to study the most likely mechanisms driving the atmosphere to the current obse…

2016 Planetary and Space Science
VenusExpress 35
A discrete chemo-dynamical model of the giant elliptical galaxy NGC 5846: dark matter fraction, internal rotation, and velocity anisotropy out to six effective radii
DOI: 10.1093/mnras/stw1931 Bibcode: 2016MNRAS.462.4001Z

Forbes, Duncan A.; Romanowsky, Aaron J.; Brodie, Jean +7 more

We construct a suite of discrete chemo-dynamical models of the giant elliptical galaxy NGC 5846. These models are a powerful tool to constrain both the mass distribution and internal dynamics of multiple tracer populations. We use Jeans models to simultaneously fit stellar kinematics within the effective radius Re, planetary nebula (PN)…

2016 Monthly Notices of the Royal Astronomical Society
eHST 35
A complete census of Herschel-detected infrared sources within the HST Frontier Fields
DOI: 10.1093/mnras/stw712 Bibcode: 2016MNRAS.459.1626R

Smail, I.; Kneib, J. -P.; Lutz, D. +16 more

We present a complete census of all Herschel-detected sources within the six massive lensing clusters of the HST Frontier Fields (HFF). We provide a robust legacy catalogue of 263 sources with Herschel fluxes, primarily based on imaging from the Herschel Lensing Survey and PEP/HerMES Key Programmes. We optimally combine Herschel, Spitzer and WISE …

2016 Monthly Notices of the Royal Astronomical Society
Herschel eHST 35
Strong constraints on a super-Eddington accretion flow: XMM-Newton observations of an intermediate-mass black hole
DOI: 10.1093/mnras/stv2319 Bibcode: 2016MNRAS.455..691J

Done, Chris; Ward, Martin; Jin, Chichuan

RX J1140.1+0307 is a Narrow Line Seyfert 1 (NLS1) with one of the lowest black hole masses known in an AGN (M ≤ 106 M). We show results from two new XMM-Newton observations, exhibiting soft 2-10 keV spectra, a strong excess at lower energies, and fast X-ray variability which is typical of this class of AGN. The soft excess c…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 35