Search Publications

ALMA observations of cold molecular gas filaments trailing rising radio bubbles in PKS 0745-191
DOI: 10.1093/mnras/stw409 Bibcode: 2016MNRAS.458.3134R

O'Connell, R. W.; Fabian, A. C.; Combes, F. +16 more

We present ALMA observations of the CO(1-0) and CO(3-2) line emission tracing filaments of cold molecular gas in the central galaxy of the cluster PKS 0745-191. The total molecular gas mass of 4.6± 0.3× 109 M_{⊙}, assuming a Galactic XCO factor, is divided roughly equally between three filaments each extending radially 3-5 kp…

2016 Monthly Notices of the Royal Astronomical Society
eHST 81
Modelling supernova line profile asymmetries to determine ejecta dust masses: SN 1987A from days 714 to 3604
DOI: 10.1093/mnras/stv2651 Bibcode: 2016MNRAS.456.1269B

Barlow, M. J.; Bevan, Antonia

The late-time optical and near-IR line profiles of many core-collapse supernovae exhibit a red-blue asymmetry as a result of greater extinction by internal dust of radiation emitted from the receding parts of the supernova ejecta. We present here a new code, DAMOCLES, that models the effects of dust on the line profiles of core-collapse supernovae…

2016 Monthly Notices of the Royal Astronomical Society
eHST 81
Dead or Alive? Long-term evolution of SN 2015bh (SNhunt275)
DOI: 10.1093/mnras/stw2253 Bibcode: 2016MNRAS.463.3894E

Brown, P. J.; Smartt, S. J.; Kotak, R. +37 more

Supernova (SN) 2015bh (or SNhunt275) was discovered in NGC 2770 on 2015 February with an absolute magnitude of Mr ∼ -13.4 mag, and was initially classified as an SN impostor. Here, we present the photometric and spectroscopic evolution of SN 2015bh from discovery to late phases (∼1 yr after). In addition, we inspect archival images of t…

2016 Monthly Notices of the Royal Astronomical Society
eHST 81
A self-consistent model for the evolution of the gas produced in the debris disc of β Pictoris
DOI: 10.1093/mnras/stw1361 Bibcode: 2016MNRAS.461..845K

Pringle, J. E.; Kral, Q.; Juhász, A. +3 more

This paper presents a self-consistent model for the evolution of gas produced in the debris disc of β Pictoris. Our model proposes that atomic carbon and oxygen are created from the photodissociation of CO, which is itself released from volatile-rich bodies in the debris disc due to grain-grain collisions or photodesorption. While the CO lasts les…

2016 Monthly Notices of the Royal Astronomical Society
Herschel 80
X-ray spectral properties of the AGN sample in the northern XMM-XXL field
DOI: 10.1093/mnras/stw753 Bibcode: 2016MNRAS.459.1602L

Shen, Yue; Nandra, Kirpal; Streblyanska, Alina +7 more

In this paper we describe and publicly release a catalogue consisting of 8445 point-like X-ray sources detected in the XMM-XXL north survey. For the 2512 AGN which have reliable spectroscopy from SDSS-III/BOSS, we present the X-ray spectral fitting which has been computed with a Bayesian approach. We have also applied an X-ray spectral stacking me…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 78
Baryon cycling in the low-redshift circumgalactic medium: a comparison of simulations to the COS-Halos survey
DOI: 10.1093/mnras/stw595 Bibcode: 2016MNRAS.459.1745F

Kollmeier, Juna A.; Davé, Romeel; Tumlinson, Jason +8 more

We analyse the low-redshift (z ≈ 0.2) circumgalactic medium (CGM) by comparing absorption-line data from the COS-Halos survey to absorption around a matched galaxy sample from two cosmological hydrodynamic simulations. The models include different prescriptions for galactic outflows, namely hybrid energy/momentum driven wind (ezw), and constant wi…

2016 Monthly Notices of the Royal Astronomical Society
eHST 78
HerMES: a search for high-redshift dusty galaxies in the HerMES Large Mode Survey - catalogue, number counts and early results
DOI: 10.1093/mnras/stw1769 Bibcode: 2016MNRAS.462.1989A

Pérez-Fournon, I.; Ivison, R. J.; Clements, D. L. +25 more

Selecting sources with rising flux densities towards longer wavelengths from Herschel/Spectral and Photometric Imaging Receiver (SPIRE) maps is an efficient way to produce a catalogue rich in high-redshift (z > 4) dusty star-forming galaxies. The effectiveness of this approach has already been confirmed by spectroscopic follow-up observations, …

2016 Monthly Notices of the Royal Astronomical Society
Herschel 78
Shining a light on galactic outflows: photoionized outflows
DOI: 10.1093/mnras/stw178 Bibcode: 2016MNRAS.457.3133C

Chisholm, John; Leitherer, Claus; Chen, Yanmei +2 more

We study the ionization structure of galactic outflows in 37 nearby, star-forming galaxies with the Cosmic Origins Spectrograph on the Hubble Space Telescope. We use the O I, Si II, Si III, and Si IV ultraviolet absorption lines to characterize the different ionization states of outflowing gas. We measure the equivalent widths, line widths, and ou…

2016 Monthly Notices of the Royal Astronomical Society
eHST 77
Deep XMM observations of Draco rule out at the 99 per cent confidence level a dark matter decay origin for the 3.5 keV line
DOI: 10.1093/mnras/stw578 Bibcode: 2016MNRAS.458.3592J

Profumo, Stefano; Jeltema, Tesla

We searched for an X-ray line at energies around 3.5 keV in deep, ∼1.6 Ms XMM-Newton observations of the dwarf spheroidal galaxy Draco. No line was found in either the Metal Oxide Semi-conductor (MOS) or the p-type/n-type semiconductor (PN) detectors. The data in this energy range are completely consistent with a single, unfolded power-law modelli…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 75
Deep Chandra observations of Pictor A
DOI: 10.1093/mnras/stv2553 Bibcode: 2016MNRAS.455.3526H

Stawarz, Ł.; Hardcastle, M. J.; Croston, J. H. +7 more

We report on deep Chandra observations of the nearby broad-line radio galaxy Pictor A, which we combine with new Australia Telescope Compact Array (ATCA) observations. The new X-ray data have a factor of 4 more exposure than observations previously presented and span a 15 yr time baseline, allowing a detailed study of the spatial, temporal and spe…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 75