Search Publications

A Very Large Telescope imaging and spectroscopic survey of the Wolf-Rayet population in NGC7793
DOI: 10.1111/j.1365-2966.2010.16659.x Bibcode: 2010MNRAS.405.2737B

Crowther, P. A.; Bibby, J. L.

We present a Very Large Telescope/Focal Reducer and Low Dispersion Spectrograph #1 (VLT/FORS1) imaging and spectroscopic survey of the Wolf-Rayet (WR) population in the Sculptor group spiral galaxy NGC7793. We identify 74 emission-line candidates from archival narrow-band imaging, from which 39 were observed with the Multi Object Spectroscopy mode…

2010 Monthly Notices of the Royal Astronomical Society
eHST 33
Radio weak gravitational lensing with VLA and MERLIN
DOI: 10.1111/j.1365-2966.2009.15836.x Bibcode: 2010MNRAS.401.2572P

Muxlow, T. W. B.; Beswick, R. J.; Hoyle, B. +2 more

We carry out an exploratory weak gravitational lensing analysis on a combined Very Large Array and Multi-Element Radio-Linked Interferometer Network radio data set: a deep (3.3µJybeam-1 rms noise) 1.4GHz image of the Hubble Deep Field-North. We measure the shear estimator distribution at this radio sensitivity for the first time, …

2010 Monthly Notices of the Royal Astronomical Society
eHST 32
Direct observation of cosmic strings via their strong gravitational lensing effect - II. Results from the HST/ACS image archive
DOI: 10.1111/j.1365-2966.2010.16562.x Bibcode: 2010MNRAS.406.2452M

Treu, Tommaso; Schrabback, Tim; Blandford, Roger D. +2 more

We have searched 4.5deg2 of archival Hubble Space Telescope/Advanced Camera for Surveys (HST/ACS) images for cosmic strings, identifying close pairs of similar, faint galaxies and selecting groups whose alignment is consistent with gravitational lensing by a long, straight string. We find no evidence for cosmic strings in five large-are…

2010 Monthly Notices of the Royal Astronomical Society
eHST 32
Observational constraints on supermassive dark stars
DOI: 10.1111/j.1745-3933.2010.00908.x Bibcode: 2010MNRAS.407L..74Z

Östlin, Göran; Rydberg, Claes-Erik; Zackrisson, Erik +6 more

Some of the first stars could be cooler and more massive than standard stellar models would suggest, due to the effects of dark matter annihilation in their cores. It has recently been argued that such objects may attain masses in the 104-107Msolar range and that such supermassive dark stars should be within reach …

2010 Monthly Notices of the Royal Astronomical Society
eHST 31
The central region of M83: massive star formation, kinematics, and the location and origin of the nucleus
DOI: 10.1111/j.1365-2966.2010.17180.x Bibcode: 2010MNRAS.408..797K

Knapen, J. H.; Sharp, R. G.; Ryder, S. D. +3 more

We report new near-IR integral field spectroscopy of the central starburst region of the barred spiral galaxy M83 obtained with Cambridge Infra-Red Panoramic Survey Spectrograph (CIRPASS) on Gemini-South, which we analyse in conjunction with GHαFaS Fabry-Perot data, an Anglo-Australian Telescope (AAT) IRIS2 Ks-band image, and near- and …

2010 Monthly Notices of the Royal Astronomical Society
eHST 31
A relativistically broadened OVIII Lyα line in the ultracompact X-ray binary 4U 0614+091
DOI: 10.1111/j.1745-3933.2010.00892.x Bibcode: 2010MNRAS.407L..11M

de Plaa, J.; Fabian, A. C.; Pinto, C. +3 more

Ultracompact X-ray binaries consist of a neutron star or black hole that accretes material from a white dwarf donor star. The ultracompact nature is expressed in very short orbital periods of less than 1 h. In the case of 4U 0614+091 oxygen-rich material from a CO or ONe white dwarf is flowing to the neutron star. This oxygen-rich disc can reflect…

2010 Monthly Notices of the Royal Astronomical Society
XMM-Newton 30
The circumnuclear environment of the peculiar galaxy NGC3310
DOI: 10.1111/j.1365-2966.2009.15934.x Bibcode: 2010MNRAS.402.1005H

Terlevich, Roberto; Terlevich, Elena; Díaz, Ángeles I. +2 more

Gas and star velocity dispersions have been derived for eight circumnuclear star-forming regions (CNSFRs) and the nucleus of the spiral galaxy NGC3310 using high-resolution spectroscopy in the blue and far red. Stellar velocity dispersions have been obtained from the CaII triplet in the near-IR, using cross-correlation techniques, while gas veloci…

2010 Monthly Notices of the Royal Astronomical Society
eHST 29
Wide-field HST/ACS images of M81: the population of compact star clusters
DOI: 10.1111/j.1365-2966.2010.16531.x Bibcode: 2010MNRAS.405.1293S

Mayya, Y. D.; Rosa-González, D.; Santiago-Cortés, M.

We study the population of compact star clusters (CSCs) in M81, using the Hubble Space Telescope/Advanced Camera for Surveys (ACS) images in the filters F435W, F606W and F814W covering, for the first time, the entire optical extent of the galaxy. Our sample contains 435 clusters of full width at half-maximum less than 10 ACS pixels (9pc). The samp…

2010 Monthly Notices of the Royal Astronomical Society
eHST 29
Determining the extragalactic extinction law with SALT - II. Additional sample
DOI: 10.1111/j.1365-2966.2010.17334.x Bibcode: 2010MNRAS.409..727F

O'Donoghue, Darragh; Buckley, David A. H.; Sefako, Ramotholo +8 more

We present new results from an ongoing programme to study the dust extragalactic extinction law in E/S0 galaxies with dust lanes with the Southern African Large Telescope (SALT) during its performance verification phase. The wavelength dependence of the dust extinction for seven galaxies is derived in six spectral bands ranging from the near-ultra…

2010 Monthly Notices of the Royal Astronomical Society
eHST 28
Central galaxy growth and feedback in the most massive nearby cool core cluster
DOI: 10.1111/j.1365-2966.2010.16718.x Bibcode: 2010MNRAS.406..354O

Böhringer, H.; Simionescu, A.; Fabian, A. C. +4 more

We present multiwavelength observations of the centre of RXCJ1504.1 - 0248 - the galaxy cluster with the most luminous and relatively nearby cool core at z ~ 0.2. Although there are several galaxies within 100kpc of the cluster core, only the brightest cluster galaxy (BCG), which lies at the peak of the X-ray emission, has blue colours and strong …

2010 Monthly Notices of the Royal Astronomical Society
XMM-Newton 28