Search Publications

Massive compact galaxies with high-velocity outflows: morphological analysis and constraints on AGN activity
DOI: 10.1093/mnras/stu636 Bibcode: 2014MNRAS.441.3417S

Moustakas, J.; Heinz, S.; Hickox, R. C. +9 more

We investigate the process of rapid star formation quenching in a sample of 12 massive galaxies at intermediate redshift (z ∼ 0.6) that host high-velocity ionized gas outflows (v > 1000 km s-1). We conclude that these fast outflows are most likely driven by feedback from star formation rather than active galactic nuclei (AGNs). We us…

2014 Monthly Notices of the Royal Astronomical Society
eHST 67
LoCuSS: hydrostatic mass measurements of the high-LX cluster sample - cross-calibration of Chandra and XMM-Newton
DOI: 10.1093/mnras/stu1267 Bibcode: 2014MNRAS.443.2342M

Smith, Graham P.; Marrone, Daniel P.; Finoguenov, Alexis +5 more

We present a consistent analysis of Chandra and XMM-Newton observations of an approximately mass-selected sample of 50 galaxy clusters at 0.15 < z < 0.3 - the `LoCuSS high-LX sample'. We apply the same analysis methods to data from both satellites, including newly developed analytic background models that predict the spatial varia…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 66
Spitzer Space Telescope spectra of post-AGB stars in the Large Magellanic Cloud - polycyclic aromatic hydrocarbons at low metallicities
DOI: 10.1093/mnras/stt2495 Bibcode: 2014MNRAS.439.1472M

Sahai, R.; Hony, S.; Ita, Yoshifusa +26 more

This paper reports variations of polycyclic aromatic hydrocarbons (PAHs) features that were found in Spitzer Space Telescope spectra of carbon-rich post-asymptotic giant branch (post-AGB) stars in the Large Magellanic Cloud (LMC). The paper consists of two parts. The first part describes our Spitzer spectral observing programme of 24 stars includi…

2014 Monthly Notices of the Royal Astronomical Society
ISO 66
On the progenitor of the Type IIP SN 2013ej in M74.
DOI: 10.1093/mnrasl/slt179 Bibcode: 2014MNRAS.439L..56F

Gal-Yam, A.; Inserra, C.; Smartt, S. J. +10 more

We use natural seeing imaging of SN 2013ej in M74 to identify a progenitor candidate in archival Hubble Space Telescope (HST) + Advanced Camera for Survey images. We find a source coincident with the supernova (SN) in the F814W filter within the total 75 mas (∼3 pc astrometric uncertainty; however, the position of the progenitor candidate in conte…

2014 Monthly Notices of the Royal Astronomical Society
eHST 65
The SLUGGS survey: the globular cluster systems of three early-type galaxies using wide-field imaging
DOI: 10.1093/mnras/stt1880 Bibcode: 2014MNRAS.437..273K

Spitler, Lee R.; Forbes, Duncan A.; Romanowsky, Aaron J. +3 more

We present the results from a wide-field imaging study of globular cluster (GC) systems in three early-type galaxies. Combinations of Subaru/Suprime-Cam, Canada-France-Hawaii Telescope/MegaCam and Hubble Space Telescope/Wide Field Planetary Camera 2/Advanced Camera for Surveys data were used to determine the GC system properties of three highly fl…

2014 Monthly Notices of the Royal Astronomical Society
eHST 65
The halo+cluster system of the Galactic globular cluster NGC 1851
DOI: 10.1093/mnras/stu1099 Bibcode: 2014MNRAS.442.3044M

Weiss, A.; Milone, A. P.; Marino, A. F. +17 more

NGC 1851 is surrounded by a stellar component that extends more than 10 times beyond the tidal radius. Although the nature of this stellar structure is not known, it has been suggested to be a sparse halo of stars or associated with a stellar stream. We analyse the nature of this intriguing stellar component surrounding NGC 1851 by investigating i…

2014 Monthly Notices of the Royal Astronomical Society
eHST 65
A z = 2.5 protocluster associated with the radio galaxy MRC 2104-242: star formation and differing mass functions in dense environments
DOI: 10.1093/mnras/stu522 Bibcode: 2014MNRAS.440.3262C

Kurk, J. D.; Rigby, E. E.; Hatch, N. A. +2 more

We present results from a narrow-band survey of the field around the high-redshift radio galaxy MRC 2104-242. We have selected Hα emitters in a 7 arcmin2 field and compared the measured number density with that of a field sample at similar redshift. We find that MRC 2104-242 lies in an overdensity of galaxies that is 8.0 ± 0.8 times the…

2014 Monthly Notices of the Royal Astronomical Society
Herschel eHST 65
A late-time view of the progenitors of five Type IIP supernovae
DOI: 10.1093/mnras/stt2131 Bibcode: 2014MNRAS.438..938M

Mattila, Seppo; Maund, Justyn R.; Reilly, Emma

The acquisition of late-time imaging is an important step in the analysis of pre-explosion observations of the progenitors of supernovae. We present late-time Hubble Space Telescope Advanced Camera for Surveys Wide-Field Channel observations of the sites of five Type IIP SNe: 1999ev, 2003gd, 2004A, 2005cs and 2006my. Observations were conducted us…

2014 Monthly Notices of the Royal Astronomical Society
eHST 64
A propeller scenario for the gamma-ray emission of low-mass X-ray binaries: the case of XSS J12270-4859
DOI: 10.1093/mnras/stt2336 Bibcode: 2014MNRAS.438.2105P

Torres, D. F.; Li, Jian; Papitto, A.

XSS J12270-4859 is the only low-mass X-ray binary (LMXB) with a proposed persistent gamma-ray counterpart in the Fermi-Large Area Telescope domain, 2FGL 1227.7-4853. Here, we present the results of the analysis of recent INTEGRAL observations, aimed at assessing the long-term variability of the hard X-ray emission, and thus the stability of the ac…

2014 Monthly Notices of the Royal Astronomical Society
INTEGRAL 64
The colour distribution of galaxies at redshift five
DOI: 10.1093/mnras/stu558 Bibcode: 2014MNRAS.440.3714R

Ferguson, H. C.; Finkelstein, S. L.; Bowler, R. A. A. +11 more

We present the results of a study investigating the rest-frame ultraviolet (UV) spectral slopes of redshift z ≈ 5 Lyman-break galaxies (LBGs). By combining deep Hubble Space Telescope imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey and Hubble Ultra-Deep Field with ground-based imaging from the UKIRT Infrared Deep Sky …

2014 Monthly Notices of the Royal Astronomical Society
eHST 63