Search Publications

Spherical models of star clusters with potential escapers
DOI: 10.1093/mnras/stz1109 Bibcode: 2019MNRAS.487..147C

Varri, Anna Lisa; Heggie, Douglas C.; Gieles, Mark +2 more

An increasing number of observations of the outer regions of globular clusters (GCs) have shown a flattening of the velocity dispersion profile and an extended surface density profile. Formation scenarios of GCs can lead to different explanations of these peculiarities, therefore the dynamics of stars in the outskirts of GCs are an important tool …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 27
K2 Ultracool Dwarfs Survey - V. High superflare rates on rapidly rotating late-M dwarfs
DOI: 10.1093/mnras/stz886 Bibcode: 2019MNRAS.486.1438P

Mullan, D. J.; Burgasser, A. J.; Stassun, K. G. +5 more

We observed strong superflares (defined as flares with energy in excess of 1033 erg) on three late-M dwarfs: 2MASS J08315742+2042213 (hereafter 2M0831+2042; M7 V), 2MASS J08371832+2050349 (hereafter 2M0837+2050; M8 V), and 2MASS J08312608+2244586 (hereafter 2M0831+2244; M9 V). 2M0831+2042 and 2M0837+2050 are members of the young (∼700 M…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 27
Age gradients throughout the Galaxy with long-period variables
DOI: 10.1093/mnras/sty3284 Bibcode: 2019MNRAS.483.3022G

Evans, N. W.; Belokurov, V.; Grady, J.

We assemble the largest sample of oxygen-rich (O-rich) Miras and associated long-period variables (LPVs) to date and highlight their importance for age dating the components of the Galaxy. Using data from the Catalina Surveys and the All Sky Automated Survey for Supernovae, we extract a clean sample of ∼2200 O-rich LPVs, stretching from the Galact…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 27
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