Search Publications

Nuclear absorption and emission in the AGN merger NGC 6240 : the hard X-ray view
DOI: 10.1093/mnras/stx1878 Bibcode: 2017MNRAS.471.3483N

Nardini, Emanuele

We present the analysis of four NuSTAR observations of the luminous infrared galaxy merger NGC 6240 , hosting a close pair of highly obscured active galactic nuclei (AGNs). Over a period of about 2 yr, the source exhibits hard X-ray variability of the order of 20 per cent, peaking around 20 keV. When the two AGNs are resolved with Chandra , column…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 20
The effect of stellar and AGN feedback on the low-redshift Lyman α forest in the Sherwood simulation suite
DOI: 10.1093/mnras/stx1648 Bibcode: 2017MNRAS.471.1056N

Viel, Matteo; Sijacki, Debora; Kim, Tae-Sun +4 more

We study the effect of different feedback prescriptions on the properties of the low-redshift (z ≤ 1.6) Lyα forest using a selection of hydrodynamical simulations drawn from the Sherwood simulation suite. The simulations incorporate stellar feedback, active galactic nuclei (AGN) feedback and a simplified scheme for efficiently modelling the low co…

2017 Monthly Notices of the Royal Astronomical Society
eHST 20
A comparison between the soft X-ray and [O III] morphologies of active galactic nuclei
DOI: 10.1093/mnras/stx1037 Bibcode: 2017MNRAS.469.2720G

Gallego, Jesús; Gómez-Guijarro, Carlos; Rodríguez-Espinosa, José Miguel +2 more

Several studies of nearby active galactic nuclei (AGNs) have shown that the soft X-ray emission presents a size and morphology resembling that of the narrow-line region (NLR) traced by [O III]. Since the NLR is mainly constituted by gas photoionized by the AGN, it seems logical to assume that this is also the primary source of the soft X-ray emiss…

2017 Monthly Notices of the Royal Astronomical Society
eHST 20
Population mixtures and searches of lensed and extended quasars across photometric surveys
DOI: 10.1093/mnras/stw3239 Bibcode: 2017MNRAS.466.3088W

Treu, Tommaso; Agnello, Adriano; Williams, Peter

Wide-field photometric surveys enable searches of rare yet interesting objects, such as strongly lensed quasars or quasars with a bright host galaxy. Past searches for lensed quasars based on their optical and near-infrared properties have relied on photometric cuts and spectroscopic preselection (as in the Sloan Quasar Lens Search), or neural net…

2017 Monthly Notices of the Royal Astronomical Society
eHST 20
Sulphur isotope mass-independent fractionation observed in comet 67P/Churyumov-Gerasimenko by Rosetta/ROSINA
DOI: 10.1093/mnras/stx2534 Bibcode: 2017MNRAS.469S.787C

Altwegg, K.; Balsiger, H.; Fuselier, S. A. +12 more

The knowledge about sulphur isotopic fractionation in volatile cometary species is limited as only measurements in five comets have been done and only for 34S/32S. The lack of information about the fractionation of 33S/32S makes it impossible to compare them with what is known from refractories. We prese…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 20
CONSERT constrains the internal structure of 67P at a few metres size scale
DOI: 10.1093/mnras/stx3132 Bibcode: 2017MNRAS.469S.805C

Plettemeier, Dirk; Kofman, Wlodek; Herique, Alain +6 more

The internal properties of cometary nuclei are the best clues to the size distribution and properties of the early planetesimals that formed the planets during the early Solar system nebula processes. The CONSERT radar was designed to probe the interior of comet 67P/Churyumov-Gerasimenko with a wavelength of about 3 m. It was successfully operated…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 20
Star formation history of And XVIII: a dwarf spheroidal galaxy in isolation
DOI: 10.1093/mnras/stw2502 Bibcode: 2017MNRAS.464.2281M

Rizzi, L.; Karachentsev, I. D.; Makarova, L. N. +2 more

We present a photometric study of the Andromeda XVIII dwarf spheroidal galaxy associated with M31, and situated well outside of the virial radius of the M31 halo. The galaxy was resolved into stars with Hubble Space Telescope/Advanced Camera for Surveys (HST/ACS) revealing the old red giant branch and red clump. With the new observational data, we…

2017 Monthly Notices of the Royal Astronomical Society
eHST 20
Models for 60 double-lined binaries containing giants
DOI: 10.1093/mnras/stx598 Bibcode: 2017MNRAS.468.3533E

Eggleton, Peter P.; Yakut, Kadri

The observed masses, radii and temperatures of 60 medium- to long-period binaries, most of which contain a cool, evolved star and a hotter less evolved one, are compared with theoretical models which include (a) core convective overshooting, (b) mass-loss, possibly driven by dynamo action as in RS CVn binaries, and (c) tidal friction, including it…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 20
Young LMC clusters: the role of red supergiants and multiple stellar populations in their integrated light and CMDs
DOI: 10.1093/mnras/stx1824 Bibcode: 2017MNRAS.471.3599A

Beasley, Michael A.; Vazdekis, Alexandre; Cerviño, Miguel +3 more

The optical integrated spectra of three Large Magellanic Cloud young stellar clusters (NGC 1984, NGC 1994 and NGC 2011) exhibit concave continua and prominent molecular bands which deviate significantly from the predictions of single stellar population (SSP) models. In order to understand the appearance of these spectra, we create a set of young s…

2017 Monthly Notices of the Royal Astronomical Society
IUE 20
On the discrepancy between asteroseismic and Gaia DR1 TGAS parallaxes
DOI: 10.1093/mnrasl/slx083 Bibcode: 2017MNRAS.470L..97G

Gontcharov, George A.; Mosenkov, Aleksandr V.

Recently, a deviation of the Gaia Tycho-Gaia Astrometric Solution (TGAS) parallaxes from the asteroseismic ones for giants was found. We show that for parallaxes ϖ < 1.5 mas it can be explained by a selection effect in favour of bright and luminous giants in the Tycho-2 and TGAS catalogues. Another explanation of this deviation seems to be vali…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 20