Search Publications

Binary deviations from single object astrometry
DOI: 10.1093/mnras/staa1148 Bibcode: 2020MNRAS.495..321P

Koposov, S. E.; Belokurov, Vasily; Penoyre, Zephyr +2 more

Most binaries are undetected. Astrometric reductions of a system using the assumption that the object moves like a single point mass can be biased by unresolved binary stars. The discrepancy between the centre of mass of the system (which moves like a point mass) and the centre of light (which is what we observe) introduces additional motion. We e…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 78
X-ray detected AGN in SDSS dwarf galaxies
DOI: 10.1093/mnras/staa040 Bibcode: 2020MNRAS.492.2268B

Birchall, Keir L.; Watson, M. G.; Aird, J.

In this work we present a robust quantification of X-ray selected AGN in local (z ≤ 0.25) dwarf galaxies (M_* ≤ 3 × 10^9 M_⊙ ). We define a parent sample of 4331 dwarf galaxies found within the footprint of both the MPA-JHU galaxy catalogue (based on SDSS DR8) and 3XMM DR7, performed a careful review of the data to remove misidentifications and pr…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 77
The R136 star cluster dissected with Hubble Space Telescope/STIS - II. Physical properties of the most massive stars in R136
DOI: 10.1093/mnras/staa2801 Bibcode: 2020MNRAS.499.1918B

Vink, Jorick S.; Brands, Sarah A.; Langer, Norbert +11 more

We present an optical analysis of 55 members of R136, the central cluster in the Tarantula Nebula of the Large Magellanic Cloud. Our sample was observed with STIS aboard the Hubble Space Telescope, is complete down to about 40 M, and includes seven very massive stars with masses over 100 M. We performed a spectroscopic anal…

2020 Monthly Notices of the Royal Astronomical Society
eHST 77
The KLEVER Survey: spatially resolved metallicity maps and gradients in a sample of 1.2 < z < 2.5 lensed galaxies
DOI: 10.1093/mnras/stz3379 Bibcode: 2020MNRAS.492..821C

Maiolino, Roberto; Cresci, Giovanni; Pettini, Max +17 more

We present near-infrared observations of 42 gravitationally lensed galaxies obtained in the framework of the KMOS Lensed Emission Lines and VElocity Review (KLEVER) Survey, a programme aimed at investigating the spatially resolved properties of the ionized gas in 1.2 < z < 2.5 galaxies by means of a full coverage of the YJ, H, and K near-inf…

2020 Monthly Notices of the Royal Astronomical Society
eHST 76
The chemical compositions of accreted and in situ galactic globular clusters according to SDSS/APOGEE
DOI: 10.1093/mnras/staa478 Bibcode: 2020MNRAS.493.3363H

Majewski, Steven R.; Beers, Timothy C.; Horta, Danny +16 more

Studies of the kinematics and chemical compositions of Galactic globular clusters (GCs) enable the reconstruction of the history of star formation, chemical evolution, and mass assembly of the Galaxy. Using the latest data release (DR16) of the SDSS/APOGEE survey, we identify 3090 stars associated with 46 GCs. Using a previously defined kinematic …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 76
Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5
DOI: 10.1093/mnras/staa1535 Bibcode: 2020MNRAS.496..695C

Cimatti, A.; Cullen, F.; McLure, R. J. +19 more

We present a sample of 151 massive (M* > 1010 M) quiescent galaxies at 2 < z < 5, based on a sophisticated Bayesian spectral energy distribution fitting analysis of the CANDELS UDS and GOODS-South fields. Our sample includes a robust sub-sample of 61 objects for which we confidently exclude low-redshift a…

2020 Monthly Notices of the Royal Astronomical Society
eHST 76
The `red supergiant problem': the upper luminosity boundary of Type II supernova progenitors
DOI: 10.1093/mnras/staa174 Bibcode: 2020MNRAS.493..468D

Beasor, Emma R.; Davies, Ben

By comparing the properties of red supergiant (RSG) supernova (SN) progenitors to those of field RSGs, it has been claimed that there is an absence of progenitors with luminosities L above log (L/L) > 5.2. This is in tension with the empirical upper luminosity limit of RSGs at log (L/L) = 5.5, a result known as the `RSG …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 76
The Galactic radial abundance gradients of C, N, O, Ne, S, Cl, and Ar from deep spectra of H II regions
DOI: 10.1093/mnras/staa1523 Bibcode: 2020MNRAS.496.1051A

Méndez-Delgado, J. E.; Arellano-Córdova, K. Z.; García-Rojas, J. +1 more

We present a reassessment of the radial abundance gradients of C, N, O, Ne, S, Cl, and Ar in the Milky Way using deep spectra of 33 H II regions gathered from the literature, covering Galactocentric distances from 6 to 17 kpc. The distances of the objects have been revised using Gaia parallaxes. We recalculate the physical conditions and ionic abu…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 75
Spiral arms in the protoplanetary disc HD100453 detected with ALMA: evidence for binary-disc interaction and a vertical temperature gradient
DOI: 10.1093/mnras/stz3090 Bibcode: 2020MNRAS.491.1335R

Dominik, C.; Benisty, M.; Stolker, T. +7 more

Scattered light high-resolution imaging of the protoplanetary disc orbiting HD100453 shows two symmetric spiral arms, possibly launched by an external stellar companion. In this paper, we present new, sensitive high-resolution (∼30 mas) Band 7 ALMA observations of this source. This is the first source where we find counterparts in the sub-mm conti…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 74
A physically motivated definition for the size of galaxies in an era of ultradeep imaging
DOI: 10.1093/mnras/staa236 Bibcode: 2020MNRAS.493...87T

Trujillo, Ignacio; Knapen, Johan H.; Chamba, Nushkia

Present-day multiwavelength deep imaging surveys allow to characterize the outskirts of galaxies with unprecedented precision. Taking advantage of this situation, we define a new physically motivated measurement of size for galaxies based on the expected location of the gas density threshold for star formation. Employing both theoretical and obser…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 74