Search Publications

Keck spectroscopic survey of strongly lensed galaxies in Abell 1703: further evidence of a relaxed, unimodal cluster
DOI: 10.1051/0004-6361/200811366 Bibcode: 2009A&A...498...37R

Jullo, E.; Richard, J.; Kneib, J. P. +2 more

Context: Strong gravitational lensing is a unique tool that can be used to accurately model the inner mass distribution of massive galaxy clusters. In particular, clusters with large Einstein radii provide a wealth of multiply imaged systems in the cluster core. Measuring the redshift of these multiple images provides strong constraints for precis…

2009 Astronomy and Astrophysics
eHST 56
Structural Parameters of Seven Small Magellanic Cloud Intermediate-Age and Old Star Clusters
DOI: 10.1088/0004-6256/138/5/1403 Bibcode: 2009AJ....138.1403G

Grebel, Eva K.; Gallagher, John S., III; Sabbi, Elena +9 more

We present structural parameters for the seven intermediate-age and old star clusters NGC 121, Lindsay 1, Kron 3, NGC 339, NGC 416, Lindsay 38, and NGC 419 in the Small Magellanic Cloud (SMC). We fit King profiles and Elson, Fall, and Freeman profiles to both surface-brightness and star-count data taken with the Advanced Camera for Surveys aboard …

2009 The Astronomical Journal
eHST 56
Detecting nanoparticles at radio frequencies: Jovian dust stream impacts on Cassini/RPWS
DOI: 10.1029/2008GL036752 Bibcode: 2009GeoRL..36.3103M

Gurnett, D. A.; Kaiser, M. L.; Meyer-Vernet, N. +1 more

We analyse wave observations by the Cassini/RPWS instrument performed during the Jovian fly-by, when the on-board dust analyser recorded dust streams which were interpreted as nanoparticles moving at about the solar wind speed. The observed wave pulses are produced by ionisation of dust grains impacting the spacecraft. Nanoparticles are detected b…

2009 Geophysical Research Letters
Cassini 56
X-Ray Substructure Studies of Four Galaxy Clusters Using XMM-Newton Data
DOI: 10.1088/0004-637X/699/2/1178 Bibcode: 2009ApJ...699.1178Z

Sarazin, Craig L.; Reiprich, Thomas H.; Finoguenov, Alexis +2 more

Mahdavi et al. find that the degree of agreement between weak lensing and X-ray mass measurements is a function of cluster radius. Numerical simulations also point out that X-ray mass proxies do not work equally well at all radii. The origin of the effect is thought to be associated with cluster mergers. Recent work presenting the cluster maps sho…

2009 The Astrophysical Journal
XMM-Newton 56
High-Resolution Timing Observations of Spin-Powered Pulsars with the AGILE Gamma-Ray Telescope
DOI: 10.1088/0004-637X/691/2/1618 Bibcode: 2009ApJ...691.1618P

Halpern, J.; Costa, E.; Mereghetti, S. +67 more

Astro-rivelatore Gamma ad Immagini LEggero (AGILE) is a small gamma-ray astronomy satellite mission of the Italian Space Agency dedicated to high-energy astrophysics launched in 2007 April. Its ~ 1 µs absolute time tagging capability coupled with a good sensitivity in the 30 MeV-30 GeV range, with simultaneous X-ray monitoring in the 18-60 k…

2009 The Astrophysical Journal
XMM-Newton 56
Relativistic Broadening of Iron Emission Lines in a Sample of Active Galactic Nuclei
DOI: 10.1088/0004-637X/702/2/1367 Bibcode: 2009ApJ...702.1367B

Brenneman, Laura W.; Reynolds, Christopher S.

We present a uniform X-ray spectral analysis of eight type-1 active galactic nuclei that have been previously observed with relativistically broadened iron emission lines. Utilizing data from the XMM-Newton European Photon Imaging Camera (EPIC-pn) we carefully model the spectral continuum, taking complex intrinsic absorption and emission into acco…

2009 The Astrophysical Journal
XMM-Newton 56
Spatially resolved mid-infrared observations of the triple system T Tauri
DOI: 10.1051/0004-6361/200811390 Bibcode: 2009A&A...502..623R

Wolf, S.; Ábrahám, P.; Henning, Th. +6 more

Aims: The aim of this study is to enhance our knowledge of the characteristics and distribution of the circumstellar dust associated with the individual components of the young hierarchical triple system T Tau.
Methods: To reach this goal, observations in the N-band (8-13 µm) with the two-telescope interferometric instrument MIDI at the …

2009 Astronomy and Astrophysics
ISO 56
A mechanism for electrostatic solitary structures in the Earth's magnetosheath
DOI: 10.1029/2009JA014306 Bibcode: 2009JGRA..114.9212L

Lakhina, G. S.; Pickett, J. S.; ViñAs, A. F. +3 more

Electrostatic solitary waves (ESWs) have been observed in the Earth's magnetosheath region by Cluster. A mechanism for the generation of these structures in terms of electron-acoustic solitons and double layers is discussed. The model simulates the magnetosheath plasma by a four-component plasma system consisting of core electrons, two counterstre…

2009 Journal of Geophysical Research (Space Physics)
Cluster 56
A binary engine fuelling HD 87643's complex circumstellar environment. Determined using AMBER/VLTI imaging
DOI: 10.1051/0004-6361/200811592 Bibcode: 2009A&A...507..317M

Waters, L. B. F. M.; Weigelt, G.; Hofmann, K. -H. +19 more

Context: The star HD 87643, exhibiting the “B[e] phenomenon”, has one of the most extreme infrared excesses for this object class. It harbours a large amount of both hot and cold dust, and is surrounded by an extended reflection nebula.
Aims: One of our major goals was to investigate the presence of a companion in HD87643. In addition, the pre…

2009 Astronomy and Astrophysics
ISO 56
EX Lupi in quiescence
DOI: 10.1051/0004-6361/200911641 Bibcode: 2009A&A...507..881S

Ábrahám, P.; Kóspál, Á.; Kun, M. +5 more

Aims: EX Lupi is the prototype of EXors, a subclass of low-mass pre-main sequence stars whose episodic eruptions are attributed to temporarily increased accretion. In quiescence the optical and near-infrared properties of EX Lup cannot be distinguished from those of normal T Tau stars. Here we investigate whether it is the circumstellar disk struc…

2009 Astronomy and Astrophysics
ISO 56