Search Publications

Modelling the evolution of a comet subsurface: implications for 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stw2371 Bibcode: 2016MNRAS.462S.146G

Guilbert-Lepoutre, Aurélie; Rosenberg, Eric D.; Prialnik, Dina +1 more

Modelling the evolution of comets is a complex task aiming at providing constraints on physical processes and internal properties that are inaccessible to observations, although they could potentially bring key elements to our understanding of the origins of these primitive objects. This field has made a tremendous step forward in the post-Giotto …

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 26
Sublimation of icy aggregates in the coma of comet 67P/Churyumov-Gerasimenko detected with the OSIRIS cameras on board Rosetta
DOI: 10.1093/mnras/stw2117 Bibcode: 2016MNRAS.462S..57G

Jorda, L.; Lamy, P. L.; Lara, L. M. +58 more

Beginning in 2014 March, the OSIRIS (Optical, Spectroscopic, and Infrared Remote Imaging System) cameras began capturing images of the nucleus and coma (gas and dust) of comet 67P/Churyumov-Gerasimenko using both the wide angle camera (WAC) and the narrow angle camera (NAC). The many observations taken since July of 2014 have been used to study th…

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 26
The Gaia spectrophotometric standard stars survey - III. Short-term variability monitoring
DOI: 10.1093/mnras/stw1886 Bibcode: 2016MNRAS.462.3616M

Jordi, C.; Figueras, F.; Marinoni, S. +14 more

We present the results of the short-term constancy monitoring of candidate Gaia Spectrophotometric Standard Stars (SPSS). We obtained time series of typically 1.24 h - with sampling periods from 1-3 min to a few hours, depending on the case - to monitor the constancy of our candidate SPSS down to 10 mmag, as required for the calibration of Gaia ph…

2016 Monthly Notices of the Royal Astronomical Society
Gaia 26
The Chandra ACIS Timing Survey Project: glimpsing a sample of faint X-ray pulsators
DOI: 10.1093/mnras/stw1897 Bibcode: 2016MNRAS.462.4371I

Sidoli, L.; Esposito, P.; Israel, G. L. +1 more

We report on the discovery of 41 new pulsating sources in the data of the Chandra Advanced CCD Imaging Spectrometer, which is sensitive to X-ray photons in the 0.3-10 keV band. The archival data of the first 15 yr of Chandra observations were retrieved and analysed by means of fast Fourier transforms, employing a peak-detection algorithm able to s…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 26
The SLUGGS survey*: exploring the globular cluster systems of the Leo II group and their global relationships
DOI: 10.1093/mnras/stw185 Bibcode: 2016MNRAS.458..105K

Spitler, Lee R.; Forbes, Duncan A.; Romanowsky, Aaron J. +6 more

We present an investigation of the globular cluster (GC) systems of NGC 3607 and NGC 3608 as part of the ongoing SLUGGS (SAGES Legacy Unifying Globulars and GalaxieS) survey. We use wide-field imaging data from the Subaru telescope in the g, r and I filters to analyse the radial density, colour and azimuthal distributions of both GC systems. With …

2016 Monthly Notices of the Royal Astronomical Society
eHST 26
Galactic Centre hypershell model for the North Polar Spurs
DOI: 10.1093/mnras/stw623 Bibcode: 2016MNRAS.459..108S

Kataoka, J.; Matsui, H.; Nakashima, S. +5 more

The bipolar-hypershell (BHS) model for the North Polar Spurs (NPS-E, -W, and Loop I) and counter southern spurs (SPS-E and -W) is revisited based on numerical hydrodynamical simulations. Propagations of shock waves produced by energetic explosive events in the Galactic Centre are examined. Distributions of soft X-ray brightness on the sky at 0.25,…

2016 Monthly Notices of the Royal Astronomical Society
Suzaku 26
Searching for intermediate-mass black holes in globular clusters with gravitational microlensing
DOI: 10.1093/mnras/stw1137 Bibcode: 2016MNRAS.460.2025K

Kains, N.; Bramich, D. M.; Sahu, K. C. +1 more

We discuss the potential of the gravitational microlensing method as a unique tool to detect unambiguous signals caused by intermediate-mass black holes in globular clusters. We select clusters near the line of sight to the Galactic bulge and the Small Magellanic Cloud, estimate the density of background stars for each of them, and carry out simul…

2016 Monthly Notices of the Royal Astronomical Society
eHST 26
Relativistic Fe Kα line study in Seyfert 1 galaxies observed with Suzaku
DOI: 10.1093/mnras/stw596 Bibcode: 2016MNRAS.458.4198M

Nandra, K.; Ponti, G.; Mantovani, G.

We present an analysis of a sample of Seyfert 1 galaxies observed with Suzaku. The aim of this work is to examine critically the evidence for a relativistic Fe Kα line in the X-ray spectra of these active galactic nuclei. The sample was compiled from those sources in which a relativistic component was missing in at least one XMM-Newton observation…

2016 Monthly Notices of the Royal Astronomical Society
Suzaku 26
The variable spin-down rate of the transient magnetar XTE J1810-197
DOI: 10.1093/mnras/stw351 Bibcode: 2016MNRAS.458.2088P

Pintore, Fabio; Mereghetti, Sandro; Esposito, Paolo +7 more

We have analysed XMM-Newton and Chandra observations of the transient magnetar XTE J1810-197 spanning more than 11 yr, from the initial phases of the 2003 outburst to the current quiescent level. We investigated the evolution of the pulsar spin period and we found evidence for two distinct regimes: during the outburst decay, dot{ν } was highly var…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 25
Solo dwarfs I: survey introduction and first results for the Sagittarius dwarf irregular galaxy
DOI: 10.1093/mnras/stw257 Bibcode: 2016MNRAS.458.1678H

Côté, P.; Battaglia, G.; Lewis, G. F. +6 more

We introduce the Solitary Local dwarfs survey (Solo), a wide-field photometric study targeting every isolated dwarf galaxy within 3 Mpc of the Milky Way. Solo is based on (u)gi multiband imaging from Canada-France-Hawaii Telescope/MegaCam for northern targets, and Magellan/Megacam for southern targets. All galaxies fainter than MV ≃ -18…

2016 Monthly Notices of the Royal Astronomical Society
eHST 25