Search Publications

Thermal modelling of water activity on comet 67P/Churyumov-Gerasimenko with global dust mantle and plural dust-to-ice ratio
DOI: 10.1093/mnras/stx1607 Bibcode: 2017MNRAS.469S.295H

Jorda, L.; Lamy, P. L.; Lara, L. M. +51 more

We perform a thermo-physical analysis on water activity of comet 67P/Churyumov-Gerasimenko (67P). The sublimation of water is assumed to occur from beneath a global, desiccated dust mantle over the irregular-shaped nucleus. The concept of two thermal models, the recipe of model formulation and the strategy of application to comet 67P are described…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 40
An infrared view of AGN feedback in a type-2 quasar: the case of the Teacup galaxy
DOI: 10.1093/mnras/stx1287 Bibcode: 2017MNRAS.470..964R

Villar-Martín, M.; Ramos Almeida, C.; Piqueras López, J. +1 more

We present near-infrared integral field spectroscopy data obtained with Very Large Telescope/Spectrograph for INtegral Field Observations in the Near Infrared (SINFONI) of 'the Teacup galaxy'. The nuclear K-band (1.95-2.45 µm) spectrum of this radio-quiet type-2 quasar reveals a blueshifted broad component of FWHM ∼ 1600-1800 km s-1

2017 Monthly Notices of the Royal Astronomical Society
eHST 39
Constraining the dark energy equation of state using Bayes theorem and the Kullback-Leibler divergence
DOI: 10.1093/mnras/stw3102 Bibcode: 2017MNRAS.466..369H

Hobson, M. P.; Lasenby, A. N.; Hee, S. +2 more

Data-driven model-independent reconstructions of the dark energy equation of state w(z) are presented using Planck 2015 era cosmic microwave background, baryonic acoustic oscillations (BAO), Type Ia supernova (SNIa) and Lyman α (Lyα) data. These reconstructions identify the w(z) behaviour supported by the data and show a bifurcation of the equatio…

2017 Monthly Notices of the Royal Astronomical Society
Planck 39
Precise surface gravities of δ Scuti stars from asteroseismology
DOI: 10.1093/mnrasl/slx117 Bibcode: 2017MNRAS.471L.140G

Reese, D. R.; Garrido, R.; Martín-Ruiz, S. +8 more

The work reported here demonstrates that it is possible to accurately determine surface gravities of δ Scuti (δ Sct) stars using the frequency content from high-precision photometry and a measurement of the parallax. Using a sample of 10 eclipsing binary systems with a δ Sct component and the unique δ Sct star discovered with a transiting planet, …

2017 Monthly Notices of the Royal Astronomical Society
Gaia 39
Reconstructing the high-energy irradiation of the evaporating hot Jupiter HD 209458b
DOI: 10.1093/mnras/stw2421 Bibcode: 2017MNRAS.464.2396L

Wheatley, Peter J.; Louden, Tom; Briggs, Kevin

The atmosphere of the exoplanet HD 209458b is undergoing sustained mass loss, believed to be caused by X-ray and extreme-ultraviolet (XUV) irradiation from its star. The majority of this flux is not directly observable due to interstellar absorption, but is required in order to correctly model the photoevaporation of the planet and photoionization…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 39
Revealing structure and evolution within the corona of the Seyfert galaxy I Zw 1
DOI: 10.1093/mnras/stx1814 Bibcode: 2017MNRAS.471.4436W

Brandt, W. N.; Kriss, G. A.; Costantini, E. +3 more

X-ray spectral timing analysis is presented of XMM-Newton observations of the narrow-line Seyfert 1 galaxy I Zwicky 1 taken in 2015 January. After exploring the effect of background flaring on timing analyses, X-ray time lags between the reflection-dominated 0.3-1.0 keV energy and continuum-dominated 1.0-4.0 keV band are measured, indicative of re…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 39
Staying away from the bar: the local dynamical signature of slow and fast bars in the Milky Way
DOI: 10.1093/mnras/stw2807 Bibcode: 2017MNRAS.465.1443M

Siebert, Arnaud; Famaey, Benoit; Bienaymé, Olivier +3 more

Both the three-dimensional density of red clump giants and the gas kinematics in the inner Galaxy indicate that the pattern speed of the Galactic bar could be much lower than previously estimated. Here, we show that such slow bar models are unable to reproduce the bimodality observed in local stellar velocity space. We do so by computing the respo…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 38
Powerful outflows in the central parsecs of the low-luminosity active galactic nucleus NGC 1386
DOI: 10.1093/mnras/stx1401 Bibcode: 2017MNRAS.470.2845R

Prieto, M. A.; Luque, R.; Müller-Sánchez, F. +3 more

Low-luminosity active galactic nuclei, I.e. L_{bol}/Ledd ∼ 10-6-10-3, constitute the bulk population of active galactic nuclei (AGNs). Powerful jets, common in these objects, are a crucial source of feedback energy-driving mass outflows into the host galaxy and the intergalactic medium. This paper reports the first…

2017 Monthly Notices of the Royal Astronomical Society
eHST 38
Measurement of CIB power spectra over large sky areas from Planck HFI maps
DOI: 10.1093/mnras/stw3112 Bibcode: 2017MNRAS.466..286M

Lagache, Guilaine; Mak, Daisy Suet Ying; Challinor, Anthony +1 more

We present new measurements of the power spectra of the cosmic infrared background (CIB) anisotropies using the Planck 2015 full-mission High frequency instrument data at 353, 545 and 857 GHz over 20 000 deg2. We use techniques similar to those applied for the cosmological analysis of Planck, subtracting dust emission at the power spect…

2017 Monthly Notices of the Royal Astronomical Society
Herschel Planck 38
MOVES - I. The evolving magnetic field of the planet-hosting star HD189733
DOI: 10.1093/mnras/stx1581 Bibcode: 2017MNRAS.471.1246F

Moutou, C.; Vidotto, A. A.; Ehrenreich, D. +9 more

HD189733 is an active K dwarf that is, with its transiting hot Jupiter, among the most studied exoplanetary systems. In this first paper of the Multiwavelength Observations of an eVaporating Exoplanet and its Star (MOVES) programme, we present a 2-yr monitoring of the large-scale magnetic field of HD189733. The magnetic maps are reconstructed for …

2017 Monthly Notices of the Royal Astronomical Society
eHST 38