Search Publications

White dwarf pollution by hydrated planetary remnants: hydrogen and metals in WD J204713.76-125908.9
DOI: 10.1093/mnras/staa2717 Bibcode: 2020MNRAS.499..171H

Hollands, Mark; Raddi, Roberto; Gänsicke, Boris T. +9 more

WD J204713.76-125908.9 is a new addition to the small class of white dwarfs with helium-dominated photospheres that exhibit strong Balmer absorption lines and atmospheric metal pollution. The exceptional abundances of hydrogen observed in these stars may be the result of accretion of water-rich rocky bodies. We obtained far-ultraviolet and optical…

2020 Monthly Notices of the Royal Astronomical Society
Gaia eHST 38
The Gaia-ESO survey: 3D NLTE abundances in the open cluster NGC 2420 suggest atomic diffusion and turbulent mixing are at the origin of chemical abundance variations
DOI: 10.1051/0004-6361/202038833 Bibcode: 2020A&A...643A.164S

Hansen, Camilla Juul; Serenelli, Aldo; Bergemann, Maria +10 more

Context. Atomic diffusion and mixing processes in stellar interiors influence the structure and the surface composition of stars. Some of these processes cannot yet be modelled from the first principles, and they require calibrations. This limits their applicability in stellar models used for studies of stellar populations and Galactic evolution. …

2020 Astronomy and Astrophysics
Gaia 38
The hunt for pulsating ultraluminous X-ray sources
DOI: 10.1093/mnras/stz3036 Bibcode: 2020MNRAS.491.1260S

Fabian, A. C.; Roberts, T. P.; Lansbury, G. B. +4 more

Motivated by the recent discoveries that six ultraluminous X-ray sources (ULXs) are powered by highly super-Eddington X-ray pulsars, we searched for additional pulsating ULX (PULX) candidates by identifying sources that exhibit long-term flux variability of at least an order of magnitude (a common feature seen in the six known PULXs, which may pot…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 38
Reproducing the Universe: a comparison between the EAGLE simulations and the nearby DustPedia galaxy sample
DOI: 10.1093/mnras/staa857 Bibcode: 2020MNRAS.494.2823T

Mosenkov, Aleksandr V.; Meidt, Sharon E.; De Looze, Ilse +17 more

We compare the spectral energy distributions (SEDs) and inferred physical properties for simulated and observed galaxies at low redshift. We exploit UV-submillimetre mock fluxes of ∼7000 z = 0 galaxies from the EAGLE suite of cosmological simulations, derived using the radiative transfer code skirt. We compare these to ∼800 observed galaxies in th…

2020 Monthly Notices of the Royal Astronomical Society
Herschel 38
The Fornax Deep Survey with VST. IX. Catalog of sources in the FDS area with an example study for globular clusters and background galaxies
DOI: 10.1051/0004-6361/202038137 Bibcode: 2020A&A...639A.136C

van de Ven, Glenn; Mieske, Steffen; Hilker, Michael +18 more

Context. A possible pathway for understanding the events and the mechanisms involved in galaxy formation and evolution is an in-depth investigation of the galactic and inter-galactic fossil sub-structures with long dynamical timescales: stars in the field and in stellar clusters.
Aims: This paper continues the Fornax Deep Survey (FDS) series.…

2020 Astronomy and Astrophysics
eHST 38
Hard X-ray cataclysmic variables
DOI: 10.1016/j.asr.2019.09.006 Bibcode: 2020AdSpR..66.1209D

Mukai, K.; de Martino, D.; Masetti, N. +2 more

Among hard X-ray Galactic sources detected with the Swift and INTEGRAL surveys, those discovered as accreting white dwarf binaries have surprisingly boosted in number in the recent years. The majority are identified as magnetic Cataclysmic Variables of the Intermediate Polar type, suggesting this subclass as an important constituent of the Galacti…

2020 Advances in Space Research
Gaia INTEGRAL 38
Are the spiral arms in the MWC 758 protoplanetary disc driven by a companion inside the cavity?
DOI: 10.1093/mnras/staa2468 Bibcode: 2020MNRAS.498..639C

Pinte, Christophe; Christiaens, Valentin; van der Marel, Nienke +4 more

Spiral arms in protoplanetary discs are thought to be linked to the presence of companions. We test the hypothesis that the double spiral arm morphology observed in the transition disc MWC 758 can be generated by an ≈10MJup companion on an eccentric orbit internal to the spiral arms. Previous studies on MWC 758 have assumed an external …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 38
Chemodynamics of green pea galaxies - I. Outflows and turbulence driving the escape of ionizing photons and chemical enrichment
DOI: 10.1093/mnras/staa851 Bibcode: 2020MNRAS.494.3541H

Amorín, R.; Pérez-Montero, E.; Vílchez, J. M. +6 more

We investigate the ionized gas kinematics, physical properties, and chemical abundances of Sloan Digital Sky Survey J142947, a Green Pea galaxy at redshift z∼ 0.17 with strong, double-peak Ly α emission and indirect evidence of Lyman continuum (LyC) leakage. Using high-dispersion spectroscopy, we perform a multicomponent analysis of emission-line …

2020 Monthly Notices of the Royal Astronomical Society
eHST 38
The surface distributions of the production of the major volatile species, H2O, CO2, CO and O2, from the nucleus of comet 67P/Churyumov-Gerasimenko throughout the Rosetta Mission as measured by the ROSINA double focusing mass spectrometer
DOI: 10.1016/j.icarus.2019.113421 Bibcode: 2020Icar..33513421C

Hansen, Kenneth C.; Altwegg, Kathrin; Rubin, Martin +12 more

The Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) suite of instruments operated throughout the over two years of the Rosetta mission operations in the vicinity of comet 67P/Churyumov-Gerasimenko. It measured gas densities and composition throughout the comet's atmosphere, or coma. Here we present two-years' worth of measuremen…

2020 Icarus
Rosetta 38
Constraining the Kilonova Rate with Zwicky Transient Facility Searches Independent of Gravitational Wave and Short Gamma-Ray Burst Triggers
DOI: 10.3847/1538-4357/abbf4c Bibcode: 2020ApJ...904..155A

Kulkarni, S. R.; Cenko, S. Bradley; Duev, Dmitry A. +34 more

The first binary neutron star merger, GW170817, was accompanied by a radioactivity-powered optical/infrared transient called a kilonova. To date, no compelling kilonova has been found in all-sky optical surveys, independently of short gamma-ray burst and gravitational-wave triggers. In this work, we searched the first 23 months of the Zwicky Trans…

2020 The Astrophysical Journal
Gaia 38