Search Publications

Detection of 6-cm radio-continuum emission from an EB (β-Lyrae type) variable star - HIP 68718
DOI: 10.1111/j.1365-2966.2007.11783.x Bibcode: 2007MNRAS.381.1027A

Filipović, M. D.; Anderson, M. W. B.

We report the 6-cm radio-continuum detection of a previously unknown radio star, HIP 68718, identified by the Hipparcos satellite as an EB or β-Lyrae type optical variable. Only five prior radio detections of this type are reported in the literature. The radio source (VLA J140402-002145) was detected at the 6σ level, with an associated <1arcsec…

2007 Monthly Notices of the Royal Astronomical Society
Hipparcos 1
Molecular content of a Type Ia supernova host galaxy at z = 0.6
DOI: 10.1111/j.1365-2966.2007.12261.x Bibcode: 2007MNRAS.381.1508M

Combes, F.; Melchior, A. -L.

We study the properties and the molecular content of the host of a Type Ia supernova (SN1997ey). This z = 0.575 host is the brightest submillimetre source of the sample of Type Ia supernova hosts observed at 450 and 850 µm by Farrah et al. Observations were performed at the Institut de Radioastronomie Millimétrique 30 m telescope (IRAM 30m) …

2007 Monthly Notices of the Royal Astronomical Society
eHST 1
The XMM-SSC survey of hard-spectrum XMM-Newton sources - I. Optically bright sources
DOI: 10.1111/j.1365-2966.2007.11857.x Bibcode: 2007MNRAS.378.1335P

Page, M. J.; Boller, Th.; Carrera, F. J. +15 more

We present optical and X-ray data for a sample of serendipitous XMM-Newton sources that are selected to have 0.5-2 versus 2-4.5 keV X-ray hardness ratios which are harder than the X-ray background. The sources have 2-4.5 keV X-ray flux >=10-14 erg cm-2 s-1, and in this paper we examine a subsample of 42 opticall…

2007 Monthly Notices of the Royal Astronomical Society
XMM-Newton 1
The SAURON project - IV. The mass-to-light ratio, the virial mass estimator and the Fundamental Plane of elliptical and lenticular galaxies
DOI: 10.1111/j.1365-2966.2005.09981.x Bibcode: 2006MNRAS.366.1126C

Krajnović, Davor; Emsellem, Eric; van de Ven, Glenn +12 more

We investigate the well-known correlations between the dynamical mass-to-light ratio (M/L) and other global observables of elliptical (E) and lenticular (S0) galaxies. We construct two-integral Jeans and three-integral Schwarzschild dynamical models for a sample of 25 E/S0 galaxies with SAURON integral-field stellar kinematics to about one effecti…

2006 Monthly Notices of the Royal Astronomical Society
eHST 991
Elemental abundance survey of the Galactic thick disc
DOI: 10.1111/j.1365-2966.2006.10148.x Bibcode: 2006MNRAS.367.1329R

Lambert, David L.; Allende Prieto, Carlos; Reddy, Bacham E.

We have performed an abundance analysis for F- and G- dwarfs of the Galactic thick-disc component. A sample of 176 nearby (d<= 150pc) thick-disc candidate stars was chosen from the Hipparcos catalogue and subjected to a high-resolution spectroscopic analysis. Using accurate radial velocities combined with the Hipparcos astrometry, kinematics (U…

2006 Monthly Notices of the Royal Astronomical Society
Hipparcos 760
The SAURON project - V. Integral-field emission-line kinematics of 48 elliptical and lenticular galaxies
DOI: 10.1111/j.1365-2966.2005.09839.x Bibcode: 2006MNRAS.366.1151S

Bacon, Roland; Krajnović, Davor; Emsellem, Eric +10 more

We present the emission-line fluxes and kinematics of 48 representative elliptical and lenticular galaxies obtained with our custom-built integral-field spectrograph, SAURON, operating on the William Herschel Telescope. Hβ, [OIII]λλ4959,5007 and [NI]λλ5198,5200 emission lines were measured using a new procedure that simultaneously fits both the st…

2006 Monthly Notices of the Royal Astronomical Society
eHST 755
The surprising magnetic topology of τ Sco: fossil remnant or dynamo output?
DOI: 10.1111/j.1365-2966.2006.10558.x Bibcode: 2006MNRAS.370..629D

Bouret, J. -C.; Donati, J. -F.; Howarth, I. D. +9 more

We report the discovery of a medium-strength (~0.5 kG) magnetic field on the young, massive star τ Sco (B0.2V), which becomes the third-hottest magnetic star known. Circularly polarized Zeeman signatures are clearly detected in observations collected mostly with the ESPaDOnS spectropolarimeter, recently installed on the 3.6-m Canada-France-Hawaii …

2006 Monthly Notices of the Royal Astronomical Society
IUE 449
An explanation for the soft X-ray excess in active galactic nuclei
DOI: 10.1111/j.1365-2966.2005.09844.x Bibcode: 2006MNRAS.365.1067C

Fabian, A. C.; Ross, R. R.; Gallo, L. +1 more

We present a large sample of type 1 active galactic nuclei (AGN) spectra taken with XMM-Newton, and fit them with both the conventional model (a power law and blackbody) and the relativistically blurred photoionized disc reflection model of Ross & Fabian. We find that the disc reflection model is a better fit. The disc reflection model success…

2006 Monthly Notices of the Royal Astronomical Society
XMM-Newton 441
The Hubble Deep Field-North SCUBA Super-map - IV. Characterizing submillimetre galaxies using deep Spitzer imaging
DOI: 10.1111/j.1365-2966.2006.10575.x Bibcode: 2006MNRAS.370.1185P

Dickinson, Mark; Daddi, Emanuele; Chary, Ranga-Ram +9 more

We present spectral energy distributions (SEDs), Spitzer colours, and infrared (IR) luminosities for 850-µm selected galaxies in the Great Observatories Origins Deep Survey Northern (GOODS-N) field. Using the deep Spitzer Legacy images and new data and reductions of the Very Large Array-Hubble Deep Field (VLA-HDF) radio data, we find statist…

2006 Monthly Notices of the Royal Astronomical Society
eHST 326
XMM-Newton observations of the brightest ultraluminous X-ray sources
DOI: 10.1111/j.1365-2966.2006.10112.x Bibcode: 2006MNRAS.368..397S

Wilms, J.; Roberts, T. P.; Stobbart, A. -M.

We present an analysis of 13 of the best quality ultraluminous X-ray source (ULX) data sets available from XMM-Newton European Photon Imaging Camera (EPIC) observations. We utilize the high signal-to-noise in these ULX spectra to investigate the best descriptions of their spectral shape in the 0.3-10keV range. Simple models of an absorbed power la…

2006 Monthly Notices of the Royal Astronomical Society
XMM-Newton 266