Search Publications

Weak- and strong-lensing analyses of the triaxial matter distribution of Abell 1689
DOI: 10.1111/j.1365-2966.2011.19274.x Bibcode: 2011MNRAS.416.3187S

Umetsu, Keiichi; Sereno, Mauro

Haloes formed in the standard Λ cold dark matter framework should follow a universal mass density profile and fit a well-defined mass-concentration relation. Lensing analyses of clusters with a large Einstein radius seem to contradict this scenario, with the massive cluster Abell 1689 being often claimed as a notable example of a highly over-conce…

2011 Monthly Notices of the Royal Astronomical Society
eHST 48
Modelling galaxy and AGN evolution in the infrared: black hole accretion versus star formation activity
DOI: 10.1111/j.1365-2966.2011.19006.x Bibcode: 2011MNRAS.416...70G

Pozzi, F.; Vignali, C.; Gruppioni, C. +1 more

We present a new backward evolution model for galaxies and active galactic nuclei (AGNs) in the infrared (IR). What is new in this model is the separate study of the evolutionary properties of different IR populations (i.e. spiral galaxies, starburst galaxies, low-luminosity AGNs, 'unobscured' type 1 AGNs and 'obscured' type 2 AGNs) defined throug…

2011 Monthly Notices of the Royal Astronomical Society
Herschel ISO 48
Simulated spectral states of active galactic nuclei and observational predictions
DOI: 10.1111/j.1365-2966.2011.18302.x Bibcode: 2011MNRAS.413.2259S

Gierliński, Marek; Siemiginowska, Aneta; Sobolewska, Małgorzata A.

Active galactic nuclei (AGN) and galactic black hole binaries (GBHs) represent two classes of accreting black holes. They both contain an accretion disc emitting a thermal radiation, and a non-thermal X-ray emitting 'corona'. GBHs exhibit state transitions, and the spectral states are characterized by different luminosity levels and shapes of the …

2011 Monthly Notices of the Royal Astronomical Society
XMM-Newton 48
The star formation history of the Large Magellanic Cloud star cluster NGC 1751
DOI: 10.1111/j.1365-2966.2011.18538.x Bibcode: 2011MNRAS.414.2204R

Goudfrooij, Paul; Kozhurina-Platais, Vera; Rubele, Stefano +2 more

The HST/ACS colour-magnitude diagrams (CMDs) of the populous Large Magellanic Cloud (LMC) star cluster NGC 1751 present both a broad main-sequence turn-off and a dual clump of red giants. We show that the latter feature is real and associate it to the first appearance of electron degeneracy in the H-exhausted cores of the cluster stars. We then ap…

2011 Monthly Notices of the Royal Astronomical Society
eHST 47
Herschel-ATLAS: statistical properties of Galactic cirrus in the GAMA-9 Hour Science Demonstration Phase Field
DOI: 10.1111/j.1365-2966.2010.17971.x Bibcode: 2011MNRAS.412.1151B

Rodighiero, G.; Ivison, R. J.; Clements, D. L. +35 more

We study the spectral energy distribution (SED) and the power spectrum of Galactic cirrus emission observed in the 14 deg2 Science Demonstration Phase field of the Herschel-ATLAS using Herschel and IRAS data from 100 to 500 µm. We compare the Spectral and Photometric Imaging Receiver (SPIRE) 250, 350 and 500 µm maps with IRA…

2011 Monthly Notices of the Royal Astronomical Society
Herschel 47
Spatially resolved kinematics of an ultracompact dwarf galaxy
DOI: 10.1111/j.1745-3933.2011.01058.x Bibcode: 2011MNRAS.414L..70F

Infante, L.; Grebel, E. K.; Hilker, M. +3 more

We present the internal kinematics of UCD3, the brightest known ultracompact dwarf galaxy (UCD) in the Fornax cluster, making this the first UCD with spatially resolved spectroscopy. Our study is based on seeing-limited observations obtained with the ARGUS Integral Field Unit of the VLT/FLAMES spectrograph under excellent seeing conditions (0.5-0.…

2011 Monthly Notices of the Royal Astronomical Society
eHST 46
An analytic model for blue straggler formation in globular clusters
DOI: 10.1111/j.1365-2966.2011.19136.x Bibcode: 2011MNRAS.416.1410L

Sills, Alison; Knigge, Christian; Leigh, Nathan

We present an analytic model for blue straggler formation in globular clusters. We assume that blue stragglers are formed only through stellar collisions and binary star evolution, and compare our predictions to observed blue straggler numbers. We can summarize our key results as follows. (1) Binary star evolution consistently dominates blue strag…

2011 Monthly Notices of the Royal Astronomical Society
eHST 46
PTF10ops - a subluminous, normal-width light curve Type Ia supernova in the middle of nowhere
DOI: 10.1111/j.1365-2966.2011.19526.x Bibcode: 2011MNRAS.418..747M

Cenko, S. B.; Bloom, J. S.; Gal-Yam, A. +26 more

PTF10ops is a Type Ia supernova (SN Ia), whose light curve and spectral properties place it outside the current SN Ia subtype classifications. Its spectra display the characteristic lines of subluminous SNe Ia, but it has a normal-width light curve with a long rise time, typical of normal-luminosity SNe Ia. The early-time optical spectra of PTF10o…

2011 Monthly Notices of the Royal Astronomical Society
eHST 46
Radio to infrared spectra of late-type galaxies with Planck and Wilkinson Microwave Anisotropy Probe data
DOI: 10.1111/j.1745-3933.2011.01108.x Bibcode: 2011MNRAS.416L..99P

Clements, D. L.; Davies, R. D.; Dickinson, C. +2 more

We use the Planck Early Release Compact Source Catalogue combined with Wilkinson Microwave Anisotropy Probe (WMAP) and other archival measurements to construct continuum spectra of three nearby dusty star-forming galaxies: Messier 82, NGC 253 and NGC 4945. We carry out a least-squares fit to the spectra using a combination of simple synchrotron, f…

2011 Monthly Notices of the Royal Astronomical Society
Planck 46
Herschel observations of the Centaurus cluster - the dynamics of cold gas in a cool core
DOI: 10.1111/j.1365-2966.2011.19634.x Bibcode: 2011MNRAS.418.2386M

Böhringer, H.; Fabian, A. C.; Combes, F. +15 more

Brightest cluster galaxies (BCGs) in the cores of galaxy clusters have distinctly different properties from other low-redshift massive ellipticals. The majority of the BCGs in cool-core clusters show signs of active star formation. We present observations of NGC 4696, the BCG of the Centaurus galaxy cluster, at far-infrared (FIR) wavelengths with …

2011 Monthly Notices of the Royal Astronomical Society
Herschel eHST 46