Search Publications

L1495 revisited: a PPMAP view of a star-forming filament
DOI: 10.1093/mnras/stz2234 Bibcode: 2019MNRAS.489..962H

Griffin, M. J.; Smith, M. W. L.; Marsh, K. A. +4 more

We have analysed the Herschel and SCUBA-2 dust continuum observations of the main filament in the Taurus L1495 star-forming region, using the Bayesian fitting procedure PPMAP. (i) If we construct an average profile along the whole length of the filament, it has FWHM ∼eq 0.087± 0.003 pc; but the closeness to previous estimates is coincidental. (ii)…

2019 Monthly Notices of the Royal Astronomical Society
Herschel 28
Through thick or thin: multiple components of the magneto-ionic medium towards the nearby H II region Sharpless 2-27 revealed by Faraday tomography
DOI: 10.1093/mnras/stz1438 Bibcode: 2019MNRAS.487.4751T

Federrath, Christoph; Gaensler, B. M.; McClure-Griffiths, N. M. +12 more

Sharpless 2-27 (Sh2-27) is a nearby H II region excited by ζOph. We present observations of polarized radio emission from 300 to 480 MHz towards Sh2-27, made with the Parkes 64 m Radio Telescope as part of the Global Magneto-Ionic Medium Survey. These observations have an angular resolution of 1.35°, and the data are uniquely sensitive to magneto-…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 28
Galaxy cluster mergers as triggers for the formation of jellyfish galaxies: case study of the A901/2 system
DOI: 10.1093/mnras/sty3422 Bibcode: 2019MNRAS.484..906R

Chies-Santos, Ana L.; Lima Neto, Gastão B.; Roman-Oliveira, Fernanda V. +4 more

The A901/2 system is a rare case of galaxy cluster interaction, in which two galaxy clusters and two smaller groups are seen in route of collision with each other simultaneously. Within each of the four substructures, several galaxies with features indicative of jellyfish morphologies have been observed. In this paper, we propose a hydrodynamic mo…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 28
The orbital anisotropy profiles of nearby globular clusters from Gaia Data Release 2
DOI: 10.1093/mnras/stz1586 Bibcode: 2019MNRAS.487.3693J

Bovy, Jo; Webb, Jeremy J.; Jindal, Abhinav

Gaia Data Release 2 provides a wealth of data to study the internal structure of nearby globular clusters (GCs). We use this data to investigate the internal kinematics of 10 nearby GCs, with a particular focus on their poorly studied outer regions. We apply a strict set of selection criteria to remove contaminating sources and create pure cluster…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 28
Detecting dark matter cores in galaxy clusters with strong lensing
DOI: 10.1093/mnras/stz1360 Bibcode: 2019MNRAS.487.1905A

Andrade, Kevin E.; Minor, Quinn; Kaplinghat, Manoj +1 more

We test the ability of strong lensing data to constrain the size of a central core in the dark matter haloes of galaxy clusters, using Abell 611 as a prototype. Using simulated data, we show that modelling a cluster halo with ellipticity in the gravitational potential can bias the inferred mass and concentration, which may bias the inferred centra…

2019 Monthly Notices of the Royal Astronomical Society
eHST 28
The ASKAP EMU Early Science Project: radio continuum survey of the Small Magellanic Cloud
DOI: 10.1093/mnras/stz2650 Bibcode: 2019MNRAS.490.1202J

Haberl, F.; Umana, G.; Filipović, M. D. +53 more

We present two new radio continuum images from the Australian Square Kilometre Array Pathfinder (ASKAP) survey in the direction of the Small Magellanic Cloud (SMC). These images are part of the Evolutionary Map of the Universe (EMU) Early Science Project (ESP) survey of the Small and Large Magellanic Clouds. The two new source lists produced from …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 28
Globular clusters formed within dark haloes I: present-day abundance, distribution, and kinematics
DOI: 10.1093/mnras/sty2701 Bibcode: 2019MNRAS.482..219C

Peng, Eric W.; Sales, Laura V.; Creasey, Peter +1 more

We explore a scenario where metal-poor globular clusters (GCs) form at the centres of their own dark matter haloes in the early Universe before reionization. This hypothesis leads to predictions about the abundance, distribution, and kinematics of GCs today that we explore using cosmological N-body simulations and analytical modelling. We find tha…

2019 Monthly Notices of the Royal Astronomical Society
eHST 28
From kpcs to the central parsec of NGC 1097: feeding star formation and a black hole at the same time
DOI: 10.1093/mnras/stz579 Bibcode: 2019MNRAS.485.3264P

Bruzual, Gustavo; Burkert, Andreas; Prieto, M. Almudena +3 more

A panchromatic view of the star-forming ring and feeding process in the central kpc of the galaxy NGC 1097 is presented. The assembled IR to UV images at ∼10 pc resolution allow us to characterize the population of circa 250 clusters in the ring and disentangle the network of filaments of dust and gas that enshroud and feed them. The ring is a pla…

2019 Monthly Notices of the Royal Astronomical Society
eHST 28
Three-dimensional dust mapping of 12 supernovae remnants in the Galactic anticentre
DOI: 10.1093/mnras/stz1940 Bibcode: 2019MNRAS.488.3129Y

Zijlstra, A.; Jiang, B. W.; Chen, B. Q. +1 more

We present three-dimensional (3D) dust mapping of 12 supernova remnants (SNRs) in the Galactic anticentre (Galactic longitude l between 150° and 210°) based on a recent 3D interstellar extinction map. The dust distribution of the regions, which cover the full extents in the radio continuum for the individual SNRs, is discussed. Four SNRs show sign…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 28
Statistical detection of a tidal stream associated with the globular cluster M68 using Gaia data
DOI: 10.1093/mnras/stz1790 Bibcode: 2019MNRAS.488.1535P

Miralda-Escudé, Jordi; Palau, Carles G.

A method to search for tidal streams and to fit their orbits based on maximum likelihood is presented and applied to the Gaia data. Tests of the method are performed showing how a simulated stream produced by tidal stripping of a star cluster is recovered when added to a simulation of the Gaia catalogue. The method can be applied to search for str…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 28