Search Publications

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
Magnetic field pile-up and draping at intermediately active comets: results from comet 67P/Churyumov-Gerasimenko at 2.0 AU
DOI: 10.1093/mnras/stw2480 Bibcode: 2016MNRAS.462S.235K

Glassmeier, K. -H.; Goetz, C.; Richter, I. +2 more

The interaction between a comet and the impinging solar wind leads to modifications of the magnetic field in the environment of a comet. Among those, one finds magnetic field pile-up and draping, which reveal properties of the interaction and are known from previous cometary spacecraft missions. This work studies the magnetic field configuration a…

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 35
The Red Sequence at Birth in the Galaxy Cluster Cl J1449+0856 at z = 2
DOI: 10.3847/2041-8213/833/2/L20 Bibcode: 2016ApJ...833L..20S

Finoguenov, A.; Cimatti, A.; Daddi, E. +10 more

We use Hubble Space Telescope/WFC3 imaging to study the red population in the IR-selected, X-ray detected, low-mass cluster Cl J1449+0856 at z = 2, one of the few bona fide established clusters discovered at this redshift, and likely a typical progenitor of an average massive cluster today. This study explores the presence and significance of an e…

2016 The Astrophysical Journal
eHST 35
Morphologic evidence of subsurface sediment mobilization and mud volcanism in Candor and Coprates Chasmata, Valles Marineris, Mars
DOI: 10.1016/j.icarus.2015.12.051 Bibcode: 2016Icar..269...23O

Okubo, Chris H.

Populations of distinctive knobs, rings and lobate structures are observed in the Candor and Coprates Chasmata regions of Mars. To interpret the formation mechanisms of these landforms, I investigate their morphologies, facies, superposition and crosscutting relationships using data from the High Resolution Imaging Science Experiment (HiRISE) and …

2016 Icarus
MEx 35
TeV Gamma-Ray Observations of the Galactic Center Ridge by VERITAS
DOI: 10.3847/0004-637X/821/2/129 Bibcode: 2016ApJ...821..129A

Pelassa, V.; Archer, A.; Benbow, W. +73 more

The Galactic Center ridge has been observed extensively in the past by both GeV and TeV gamma-ray instruments revealing a wealth of structure, including a diffuse component and the point sources G0.9+0.1 (a composite supernova remnant) and Sgr A* (believed to be associated with the supermassive black hole located at the center of our Galaxy). Prev…

2016 The Astrophysical Journal
XMM-Newton 35