Search Publications

Proper motions and kinematics of selected bulge globular clusters
DOI: 10.1093/mnras/stv748 Bibcode: 2015MNRAS.450.3270R

Bonfanti, A.; Bica, E.; Barbuy, B. +2 more

We computed proper motions of a selected sample of globular clusters projected on the central bulge, employing CCD images gathered along the last 25 yr at the ESO-New Technology Telescope, ESO-Danish and Hubble Space Telescope telescopes. We presented a method to derive their proper motions, and a set of coordinate transformations to obtain 3D Gal…

2015 Monthly Notices of the Royal Astronomical Society
eHST 49
Early Science with the Large Millimeter Telescope: CO and [C II] Emission in the z = 4.3 AzTEC J095942.9+022938 (COSMOS AzTEC-1)
DOI: 10.1093/mnras/stv1963 Bibcode: 2015MNRAS.454.3485Y

Iono, D.; Pope, A.; Terlevich, E. +27 more

Measuring redshifted CO line emission is an unambiguous method for obtaining an accurate redshift and total cold gas content of optically faint, dusty starburst systems. Here, we report the first successful spectroscopic redshift determination of AzTEC J095942.9+022938 (`COSMOS AzTEC-1'), the brightest 1.1 mm continuum source found in the AzTEC/Ja…

2015 Monthly Notices of the Royal Astronomical Society
Herschel eHST 48
Hubble Frontier Field free-form mass mapping of the massive multiple-merging cluster MACSJ0717.5+3745
DOI: 10.1093/mnras/stv1168 Bibcode: 2015MNRAS.451.3920D

Broadhurst, Tom; Zheng, Wei; Zitrin, Adi +4 more

We examine the latest data on the cluster MACSJ0717.5+3745 from the Hubble Frontier Fields campaign. The critically lensed area is the largest known of any lens and very irregular making it a challenge for parametric modelling. Using our free-form method we obtain an accurate solution, identify here many new sets of multiple images, doubling the n…

2015 Monthly Notices of the Royal Astronomical Society
eHST 48
A powerful double radio relic system discovered in PSZ1 G108.18-11.53: evidence for a shock with non-uniform Mach number?
DOI: 10.1093/mnras/stv1873 Bibcode: 2015MNRAS.453.3483D

van Weeren, R. J.; Bonafede, A.; Brüggen, M. +5 more

Diffuse radio emission in the form of radio haloes and relics has been found in a number of merging galaxy clusters. These structures indicate that shock and turbulence associated with the merger accelerate electrons to relativistic energies. We report the discovery of a radio relic + radio halo system in PSZ1 G108.18-11.53 (z = 0.335). This clust…

2015 Monthly Notices of the Royal Astronomical Society
Planck 47
The 2MIG isolated AGNs - I. General and multiwavelength properties of AGNs and host galaxies in the northern sky
DOI: 10.1093/mnras/stu2556 Bibcode: 2015MNRAS.447.2209P

Babyk, Iu.; Sawangwit, U.; Klimanov, S. +2 more

The host isolated galaxies with active galactic nuclei (AGNs) are unique for recognizing their internal multiwavelength properties and physical parameters of accretion on the supermassive black holes outside of the environment. For detaching these effects, we studied the galaxy sample obtained by cross-matching the 2MIG (2MASS isolated galaxy) cat…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 46
Stellar models of multiple populations in globular clusters - I. The main sequence of NGC 6752
DOI: 10.1093/mnras/stu2170 Bibcode: 2015MNRAS.446.1641D

Conroy, Charlie; Dotter, Aaron; Milone, A. P. +3 more

We present stellar atmosphere and evolution models of main-sequence stars in two stellar populations of the Galactic globular cluster NGC 6752. These populations represent the two extremes of light-element abundance variations in the cluster. NGC 6752 is a benchmark cluster in the study of multiple stellar populations because of the rich array of …

2015 Monthly Notices of the Royal Astronomical Society
eHST 46
The most powerful flaring activity from the NLSy1 PMN J0948+0022
DOI: 10.1093/mnras/stu2251 Bibcode: 2015MNRAS.446.2456D

Larsson, J.; Fortin, P.; Benbow, W. +73 more

We report on multifrequency observations performed during 2012 December-2013 August of the first narrow-line Seyfert 1 galaxy detected in γ-rays, PMN J0948+0022 (z = 0.5846). A γ-ray flare was observed by the Large Area Telescope on board Fermi during 2012 December-2013 January, reaching a daily peak flux in the 0.1-100 GeV energy range of (155 ± …

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 46
UNIMAP: a generalized least-squares map maker for Herschel data
DOI: 10.1093/mnras/stu2453 Bibcode: 2015MNRAS.447.1471P

Elia, Davide; Molinari, Sergio; Pezzuto, Stefano +5 more

The Herschel space telescope hosts two infrared photometers having an unprecedented resolution, sensitivity and dynamic range. The map making, i.e. the formation of sky images from the instruments' data, is critical for the full exploitation of the satellite and is a difficult task, since the readouts are affected by several disturbances, most not…

2015 Monthly Notices of the Royal Astronomical Society
Herschel 45
Multiwavelength observations of the transitional millisecond pulsar binary XSS J12270-4859
DOI: 10.1093/mnras/stv2109 Bibcode: 2015MNRAS.454.2190D

Belloni, T.; de Martino, D.; Rea, N. +7 more

We present an analysis of X-ray, ultraviolet and optical/near-IR photometric data of the transitional millisecond pulsar binary XSS J12270-4859, obtained at different epochs after the transition to a rotation-powered radio pulsar state. The observations, while confirming the large-amplitude orbital modulation found in previous studies after the st…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 45
The radiative efficiency of a radiatively inefficient accretion flow
DOI: 10.1093/mnras/stv465 Bibcode: 2015MNRAS.449.2803D

Messenger, C.; Patruno, A.; D'Angelo, C. R. +1 more

A recent joint XMM-Newton/Nuclear Spectroscopic Telescope Array (NuSTAR) observation of the accreting neutron star Cen X-4 (LX ∼ 1033 erg s-1) revealed a hard power-law component (Γ ∼ 1-1.5) with a relatively low cut-off energy (∼10 keV), suggesting bremsstrahlung emission. The physical requirements for bremsstrahl…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 45