Search Publications

Star-forming accretion flows and the low-luminosity nuclei of giant elliptical galaxies
DOI: 10.1111/j.1365-2966.2005.09364.x Bibcode: 2005MNRAS.362..983T

Tan, Jonathan C.; Blackman, Eric G.

The luminosities of the centres of nearby elliptical galaxies are very low compared to models of thin disc accretion on to their black holes at the Bondi rate, typically a few hundredths to a few tenths of a solar mass per year. This has motivated models of inefficiently radiated accretion that invoke weak electron-ion thermal coupling, and/or inh…

2005 Monthly Notices of the Royal Astronomical Society
eHST 39
Mid-infrared imaging of NGC 1068 with VISIR at the Very Large Telescope
DOI: 10.1111/j.1745-3933.2005.00064.x Bibcode: 2005MNRAS.363L...1G

Pantin, E.; Alloin, D.; Galliano, E. +1 more

High-resolution mid-infrared (MIR) images of the central region of NGC 1068 have been obtained with VISIR, the multi-mode MIR instrument recently installed at the European Southern Observatory Very Large Telescope on Paranal. A map of the emission at 12.8 µm with increased sensitivity over the central 8 × 8 arcsec2 area is discuss…

2005 Monthly Notices of the Royal Astronomical Society
eHST 39
On the evolutionary status of early-type galaxies in clusters at z~ 0.2 - I. The Fundamental Plane
DOI: 10.1111/j.1365-2966.2005.08779.x Bibcode: 2005MNRAS.358..233F

Smail, Ian; Davies, Roger L.; Bower, Richard G. +2 more

We investigate a spectroscopic sample of 48 early-type galaxies in the rich cluster Abell 2390 at z= 0.23 and 48 early-type galaxies from a previously published survey of Abell 2218 at z= 0.18. The spectroscopic data of A2390 are based on multi-object spectroscopy using the multi-object spectrograph for Calar Alto at the 3.5-m telescope on Calar A…

2005 Monthly Notices of the Royal Astronomical Society
eHST 39
A study of two post-common envelope binary systems
DOI: 10.1111/j.1365-2966.2005.08898.x Bibcode: 2005MNRAS.359..315E

Maxted, P. F. L.; Exter, K. M.; Napiwotzki, R. +2 more

We present intermediate-resolution, phase-resolved spectra of the close-binary systems EC 11575-1845 and V664 Cas, the central star of the planetary nebula HFG 1. Both systems have a very rich emission-line spectrum originating from the face of the cool star, which is irradiated by the hot subdwarf star. The HI emission lines are wide, consistent …

2005 Monthly Notices of the Royal Astronomical Society
IUE 38
An X-ray emission-line spectrum of Nova V382Velorum 1999
DOI: 10.1111/j.1365-2966.2005.09664.x Bibcode: 2005MNRAS.364.1015N

Schmitt, J. H. M. M.; Ness, J. -U.; Jordan, C. +2 more

We report on the analysis of an X-ray grating spectrum of the Classical Nova V382Vel (1999), obtained with the Low Energy Transmission Grating (LETG)+HRC-S instrument onboard Chandra, which shows emission lines dominating over any continuum. Lines of Si, Mg, Ne, O, N and C are identified, but no Fe lines are detected. The total luminosity in the l…

2005 Monthly Notices of the Royal Astronomical Society
eHST 38
X-ray observations of the edge-on star-forming galaxy NGC 891 and its supernova SN1986J
DOI: 10.1111/j.1365-2966.2005.09336.x Bibcode: 2005MNRAS.362..581T

Stevens, Ian R.; Raychaudhury, Somak; Temple, Rowan F.

We present XMM-Newton observations of NGC 891, a nearby edge-on spiral galaxy. We analyse the extent of the diffuse emission emitted from the disc of the galaxy, and find that it has a single-temperature profile with best-fitting temperature of 0.26 keV, though the fit of a dual-temperature plasma with temperatures of 0.08 and 0.30 keV is also acc…

2005 Monthly Notices of the Royal Astronomical Society
XMM-Newton 37
The connection between ultraviolet and X-ray outflows in active galactic nuclei: the case of PDS 456
DOI: 10.1111/j.1745-3933.2005.00038.x Bibcode: 2005MNRAS.360L..25O

Simpson, Chris; O'Brien, Paul T.; Reeves, James N. +1 more

High-velocity outflows from active galactic nuclei are a well-known phenomenon in terms of the broad absorption lines seen in the ultraviolet/optical. More recently, similar, possibly related, outflows have been reported in the X-ray. The most extreme example is seen in the nearby, luminous QSO PDS 456, which displays a massive, high-velocity (500…

2005 Monthly Notices of the Royal Astronomical Society
eHST 37
Spatially resolved spectroscopy of the E+A galaxies in the z= 0.32 cluster AC 114
DOI: 10.1111/j.1365-2966.2005.08983.x Bibcode: 2005MNRAS.359.1421P

Kuntschner, Harald; Bekki, Kenji; Colless, Matthew +5 more

We present spatially resolved intermediate-resolution spectroscopy of a sample of 12 E+A galaxies in the z= 0.32 rich galaxy cluster AC 114, obtained with the FLAMES multi-integral field unit system on the Very Large Telescope (VLT) of the European Southern Observatory. Previous integrated spectroscopy of all these galaxies by Couch & Sharples…

2005 Monthly Notices of the Royal Astronomical Society
eHST 37
A Chandra observation of the X-ray environment and jet of 3C 296
DOI: 10.1111/j.1365-2966.2005.08765.x Bibcode: 2005MNRAS.358..843H

Hardcastle, M. J.; Birkinshaw, M.; Worrall, D. M. +2 more

We have observed the twin-jet radio galaxy 3C 296 with Chandra. X-ray emission is detected from the nucleus, from the inner parts of the radio jet and from a small-scale thermal environment around the jet deceleration region. As we have found in previous observations of other twin-jet radio galaxies, the X-ray jet and a steep pressure gradient in …

2005 Monthly Notices of the Royal Astronomical Society
eHST 36
Submillimetre detection of a high-redshift type 2 QSO
DOI: 10.1111/j.1365-2966.2004.08600.x Bibcode: 2005MNRAS.356.1571M

Dunlop, J. S.; Rigopoulou, D.; Tozzi, P. +6 more

We report on the first SCUBA detection of a type 2 QSO at z= 3.660 in the Chandra Deep Field South. This source is X-ray-absorbed, shows only narrow emission lines in the optical spectrum and is detected in the submillimetre: it is the ideal candidate in an evolution scheme for active galactic nuclei (AGN) (e.g. Fabian 1999; Page et al. 2004) of a…

2005 Monthly Notices of the Royal Astronomical Society
eHST 36