Search Publications

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
Evidence for magnetic field compression in shocks within the jet of V404 Cyg
DOI: 10.1093/mnras/stw2171 Bibcode: 2016MNRAS.463.1822S

Covino, S.; Russell, D. M.; Fender, R. P. +3 more

We present optical and near-IR linear polarimetry of V404 Cyg during its 2015 outburst and in quiescence. We obtained time-resolved r'-band polarimetry when the source was in outburst, near-IR polarimetry when the source was near quiescence and multiple waveband optical polarimetry later in quiescence. The optical-to-near-IR linear pola…

2016 Monthly Notices of the Royal Astronomical Society
INTEGRAL 34
Free-free and H42α emission from the dusty starburst within NGC 4945 as observed by ALMA
DOI: 10.1093/mnras/stw1659 Bibcode: 2016MNRAS.463..252B

Dickinson, C.; Bendo, G. J.; Karim, A. +3 more

We present observations of the 85.69 GHz continuum emission and H42α line emission from the central 30 arcsec within NGC 4945. Both sources of emission originate from nearly identical structures that can be modelled as exponential discs with scalelengths of ∼2.1 arcsec (or ∼40 pc). An analysis of the spectral energy distribution based on combining…

2016 Monthly Notices of the Royal Astronomical Society
Herschel 34
Galaxy Zoo: Mergers - Dynamical models of interacting galaxies
DOI: 10.1093/mnras/stw649 Bibcode: 2016MNRAS.459..720H

Keel, William C.; Parrish, Michael; Smith, Arfon M. +6 more

The dynamical history of most merging galaxies is not well understood. Correlations between galaxy interaction and star formation have been found in previous studies, but require the context of the physical history of merging systems for full insight into the processes that lead to enhanced star formation. We present the results of simulations tha…

2016 Monthly Notices of the Royal Astronomical Society
eHST 34
H-ATLAS: a candidate high redshift cluster/protocluster of star-forming galaxies
DOI: 10.1093/mnras/stw1224 Bibcode: 2016MNRAS.461.1719C

Pérez-Fournon, I.; Valtchanov, I.; Ivison, R. J. +33 more

We investigate the region around the Planck-detected z = 3.26 gravitationally lensed galaxy HATLAS J114637.9-001132 (hereinafter HATLAS12-00) using both archival Herschel data from the H-ATLAS survey and using submm data obtained with both LABOCA and SCUBA2. The lensed source is found to be surrounded by a strong overdensity of both Herschel-SPIRE…

2016 Monthly Notices of the Royal Astronomical Society
Herschel Planck 34
Gas outflow and dust transport of comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stx332 Bibcode: 2016MNRAS.462S.533L

Bertaux, Jean-Loup; Da Deppo, Vania; Naletto, Giampiero +46 more

Because of the diurnal thermal cycle and the irregular shape of the nucleus, gas outflow of comet 67P/Churyumov-Gerasimenko could be highly anisotropic as indicated by the colliminated dust jet structures on the sunlit side. Based on the OSIRIS imaging observations of the outgassing effect, a simple model of surface sublimation can be constructed …

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 34
A possible Chandra and Hubble Space Telescope detection of extragalactic WHIM towards PG 1116+215
DOI: 10.1093/mnras/stw285 Bibcode: 2016MNRAS.457.4236B

Bonamente, M.; Tempel, E.; Nevalainen, J. +4 more

We have analysed Chandra low energy transmission grating and XMM-Newton Reflection Grating Spectrometer (RGS) spectra towards the z = 0.177 quasar PG 1116+215, a sightline that is rendered particularly interesting by the Hubble Space Telescope (HST) detection of several O VI and H I broad Lyman α absorption (BLA) lines that may be associated with …

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 34