Search Publications

Angular momentum of z ∼ 1.5 galaxies and their local analogues with adaptive optics
DOI: 10.1093/mnras/stz750 Bibcode: 2019MNRAS.485.5700S

Glazebrook, Karl; Fisher, Deanne B.; Obreschkow, Danail +9 more

We present stellar specific angular momentum j* measurements of two z ∼ 1.5 galaxies in the KGES sample and 12 DYNAMO z ∼ 0.1 analogues of high-redshift galaxies. We combine natural seeing integral field spectroscopic data to trace line emission out to high multiples of effective radius re, with adaptive optics assisted Keck/…

2019 Monthly Notices of the Royal Astronomical Society
eHST 16
Light element variations within the different age-metallicity populations in the nucleus of the Sagittarius dwarf
DOI: 10.1093/mnrasl/slz149 Bibcode: 2019MNRAS.490L..67S

Cadelano, Mario; Dalessandro, Emanuele; Sills, Alison +2 more

The cluster M54 lies at the centre of the Sagittarius dwarf spheroidal galaxy, and therefore may be the closest example of a nuclear star cluster. Either in situ star formation, inspiralling globular clusters, or a combination have been invoked to explain the wide variety of stellar sub-populations in nuclear star clusters. Globular clusters are k…

2019 Monthly Notices of the Royal Astronomical Society
eHST 16
Image simulations for gravitational lensing with SKYLENS
DOI: 10.1093/mnras/sty2737 Bibcode: 2019MNRAS.482.2823P

Plazas, A. A.; Meneghetti, M.; Rhodes, J. +1 more

We present the latest version of the ray-tracing simulation code SKYLENS, which can be used to develop image simulations that reproduce strong lensing observations by any mass distribution with a high level of realism. Improvements of the code with respect to previous versions include the implementation of the multilens plane formalism, the use of…

2019 Monthly Notices of the Royal Astronomical Society
eHST 16
Two kinematically distinct old globular cluster populations in the Large Magellanic Cloud
DOI: 10.1093/mnrasl/sly240 Bibcode: 2019MNRAS.484L..19P

Piatti, Andrés E.; Cantat-Gaudin, Tristan; Alfaro, Emilio J.

We report results of proper motions of 15 known Large Magellanic Cloud (LMC) old globular clusters (GCs) derived from the Gaia DR2 data sets. When these mean proper motions are gathered with existent radial velocity measurements to compose the GCs' velocity vectors, we found that the projection of the velocity vectors on to the LMC plane and those…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 16
Star formation quenching imprinted on the internal structure of naked red nuggets
DOI: 10.1093/mnras/stz1544 Bibcode: 2019MNRAS.487.4939M

van de Ven, Glenn; Yıldırım, Akın; Martín-Navarro, Ignacio

The formation and assembly process of massive galaxies is a combination of two phases: an initial in-situ-dominated one followed by an ex-situ-dominated evolution. Separating these two contributions is therefore crucial to understand the baryonic cycle within massive haloes. A recently discovered population of so-called naked red nuggets, galaxies…

2019 Monthly Notices of the Royal Astronomical Society
eHST 16
Free-form GRALE reconstruction of Abell 2744: robustness of uncertainties against changes in lensing data
DOI: 10.1093/mnras/stz1950 Bibcode: 2019MNRAS.488.3251S

Medezinski, Elinor; Okabe, Nobuhiro; Liesenborgs, Jori +2 more

Abell 2744, a massive Hubble Frontier Fields merging galaxy cluster with many multiple images in the core has been the subject of many lens inversions using different methods. While most existing studies compare various inversion methods, we focus on a comparison of reconstructions that use different input lensing data. Since the quantity and qual…

2019 Monthly Notices of the Royal Astronomical Society
eHST 16
Limits on a population of collisional-triples as progenitors of Type-Ia supernovae
DOI: 10.1093/mnras/stz2535 Bibcode: 2019MNRAS.490..657H

Maoz, Dan; Hallakoun, Na'ama

The progenitor systems of Type-Ia supernovae (SNe Ia) are yet unknown. The collisional-triple SN Ia progenitor model posits that SNe Ia result from head-on collisions of binary white dwarfs (WDs), driven by dynamical perturbations by the tertiary stars in mild-hierarchical triple systems. To reproduce the Galactic SN Ia rate, at least ∼30-55 per c…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 16
Kinetic Alfvén solitary waves in a plasma with two-temperature superthermal electron populations: the case of Saturn's magnetosphere
DOI: 10.1093/mnras/stz1221 Bibcode: 2019MNRAS.486.5504S

Singh, Manpreet; Saini, N. S.; Kourakis, I.

Thanks to the evidence provided by the Cassini spacecraft mission, it is now established that Saturn's magnetospheric plasma consists of various types of positive ions, as well as two distinct populations of electrons, at different temperatures. The electron population energy distributions are characterized by long suprathermal tails and have been…

2019 Monthly Notices of the Royal Astronomical Society
Cassini 16
The 11 yr of low activity of the magnetar XTE J1810-197
DOI: 10.1093/mnras/sty3378 Bibcode: 2019MNRAS.483.3832P

Pintore, Fabio; Mereghetti, Sandro; Esposito, Paolo +5 more

In 2003, the magnetar XTE J1810-197 started an outburst that lasted until early 2007. In the following 11 yr, the source stayed in a quiescent/low-activity phase. XTE J1810-197 is one of the closest magnetars, hence its X-ray properties can be studied in detail even in quiescence and an extended monitoring has been carried out to study its long-te…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 16
Comprehensive abundance analysis of red giants in the open clusters Stock 2, NGC 2168, 6475, 6991, and 7762
DOI: 10.1093/mnras/stz468 Bibcode: 2019MNRAS.485.3623R

Lambert, David L.; Reddy, Arumalla B. S.

We have analysed high-dispersion Echelle spectra (R = 60 000) of red giant members of five open clusters to derive abundances for many elements from Na to Eu. The [Fe/H] values are -0.06 ± 0.03 for Stock 2, -0.11 ± 0.03 for NGC 2168, -0.01 ± 0.03 for NGC 6475, 0.00 ± 0.03 for NGC 6991, and -0.07 ± 0.03 for NGC 7662. Sodium is enriched in the giant…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 16