Search Publications

The geometric challenge of testing gravity with wide binaries
DOI: 10.1093/mnras/sty3109 Bibcode: 2019MNRAS.482.5018E

El-Badry, Kareem

Wide binaries provide promising laboratories for testing general relativity (GR) in the low-acceleration regime. Recent observational studies have found that the difference in the proper motions and/or radial velocities of the components of nearby wide binaries appear larger than predicted by Kepler's laws, indicating a potential breakdown of GR a…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 27
Helium enrichment in intermediate-age Magellanic Clouds clusters: towards an ubiquity of multiple stellar populations?
DOI: 10.1093/mnras/stz378 Bibcode: 2019MNRAS.484.5236C

Martocchia, S.; Salaris, M.; Bastian, N. +1 more

Intermediate-age star clusters in the Magellanic Clouds harbour signatures of the multiple stellar populations long thought to be restricted to old globular clusters. We compare synthetic horizontal branch models with Hubble Space Telescope photometry of clusters in the Magellanic Clouds, with age between ∼2 and ∼10 Gyr, namely NGC 121, Lindsay 1,…

2019 Monthly Notices of the Royal Astronomical Society
eHST 27
A new study of the variable star population in the Hercules globular cluster (M13; NGC 6205)
DOI: 10.1093/mnras/stz642 Bibcode: 2019MNRAS.486.2791D

Arellano Ferro, A.; Calderón, J. H.; Lázaro, C. +4 more

We present the results from VI CCD time-series photometry of the globular cluster M13 (NGC 6205). From the Fourier decomposition of the light curves of RRab and RRc stars we found an average metallicity of [Fe/H]zw = -1.58 ± 0.09. The distance to the cluster was estimated as 7.1 ± 0.1 kpc from independent methods related to the variable star famil…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 27
60Fe in core-collapse supernovae and prospects for X-ray and gamma-ray detection in supernova remnants
DOI: 10.1093/mnras/stz536 Bibcode: 2019MNRAS.485.4287J

Safi-Harb, Samar; Fryer, Chris L.; Mumpower, Matthew R. +6 more

We investigate 60Fe in massive stars and core-collapse supernovae focussing on uncertainties that influence its production in 15, 20, and 25 M stars at solar metallicity. We find that the 60Fe yield is a monotonic increasing function of the uncertain 59Fe(n, γ)60Fe cross-section and that a fa…

2019 Monthly Notices of the Royal Astronomical Society
INTEGRAL 27
WASP-166b: a bloated super-Neptune transiting a V = 9 star
DOI: 10.1093/mnras/stz1903 Bibcode: 2019MNRAS.488.3067H

Bouchy, F.; Queloz, D.; Hellier, Coel +21 more

We report the discovery of WASP-166b, a super-Neptune planet with a mass of 0.1 MJup (1.9 MNep) and a bloated radius of 0.63 RJup. It transits a V = 9.36, F9V star in a 5.44-d orbit that is aligned with the stellar rotation axis (sky-projected obliquity angle λ = 3 ± 5 deg). Variations in the radial-velocity measur…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 27
Smoking gun of the dynamical processing of solar-type field binary stars
DOI: 10.1093/mnras/stz2274 Bibcode: 2019MNRAS.490..550L

Liu, Chao

I investigate the binarity properties of field stars using more than 50 000 main-sequence stars with stellar mass from 0.4 to 0.85 M observed by LAMOST and Gaia in the solar neighbourhood. By adopting a power-law shape for the mass-ratio distribution with a power index of γ, I conduct a hierarchical Bayesian model to derive the binary …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 27
HIDES spectroscopy of bright detached eclipsing binaries from the Kepler field - III. Spectral analysis, updated parameters and new systems
DOI: 10.1093/mnras/sty3528 Bibcode: 2019MNRAS.484..451H

Kambe, E.; Pigulski, A.; Maehara, H. +5 more

We present the latest results of our spectroscopic observations and refined modelling of a sample of detached eclipsing binaries, selected from the Kepler Eclipsing Binary Catalog, that are also double-lined spectroscopic binaries (SB2s). New high-resolution spectra obtained with the HIgh-Dispersion Echelle Spectrograph (HIDES), attached to the 1.…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 27
The O star hinterland of the Galactic starburst, NGC 3603
DOI: 10.1093/mnras/stz864 Bibcode: 2019MNRAS.486.1034D

Monguió, M.; Wright, N. J.; Drew, J. E.

The very bright and compact massive young cluster, NGC 3603, has been cited as an example of a starburst in the Milky Way and compared with the much-studied R136/30 Doradus region in the Large Magellanic Cloud. Here we build on the discovery by Mohr-Smith et al. of a large number of reddened O stars around this cluster. We construct a list of 288 …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 27
Tracking the variable jets of V404 Cygni during its 2015 outburst
DOI: 10.1093/mnras/sty2853 Bibcode: 2019MNRAS.482.2950T

Altamirano, D.; Bremer, M.; Russell, D. M. +14 more

We present multifrequency monitoring observations of the black hole X-ray binary V404 Cygni throughout its 2015 June outburst. Our data set includes radio and mm/sub-mm photometry, taken with the Karl G. Jansky Very Large Array, Arc-Minute MicroKelvin Imager Large Array, Sub-millimeter Array, James Clerk Maxwell Telescope, and the Northern Extende…

2019 Monthly Notices of the Royal Astronomical Society
INTEGRAL 27
Physical properties of the X-ray gas as a dynamical diagnosis for galaxy clusters
DOI: 10.1093/mnras/stz148 Bibcode: 2019MNRAS.484.2807L

Durret, F.; Lopes, P. A. A.; Laganá, T. F.

We analysed XMM-Newton EPIC data for 53 galaxy clusters. Through 2D spectral maps, we provide the most detailed and extended view of the spatial distribution of temperature (kT), pressure (P), entropy (S), and metallicity (Z) of galaxy clusters to date with the aim of correlating the dynamical state of the system to six cool-core (CC) diagnoses fr…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 27