Search Publications

Unveiling the nature of INTEGRAL objects through optical spectroscopy. VI. A multi-observatory identification campaign
DOI: 10.1051/0004-6361:20079332 Bibcode: 2008A&A...482..113M

Palazzi, E.; Minniti, D.; Masetti, N. +18 more

Using 8 telescopes in the northern and southern hemispheres, plus archival data from two on-line sky surveys, we performed a systematic optical spectroscopic study of 39 putative counterparts of unidentified or poorly studied INTEGRAL sources in order to determine or at least better assess their nature. This was implemented within the framework of…

2008 Astronomy and Astrophysics
INTEGRAL XMM-Newton 109
On the detectability of Lyα emission in star forming galaxies. The role of dust
DOI: 10.1051/0004-6361:200809527 Bibcode: 2008A&A...488..491A

Östlin, G.; Hayes, M.; Mas-Hesse, J. M. +2 more

Context: Lyman-alpha (Lyα) radiation is now widely used to investigate the galaxy formation and evolution in the high redshift universe. However, without a rigorous understanding of the processes regulating the Lyα escape fraction, physical interpretations of high-z observations remain questionable.
Aims: We examine six nearby star forming gal…

2008 Astronomy and Astrophysics
eHST 109
Late Amazonian glaciation at the dichotomy boundary on Mars: Evidence for glacial thickness maxima and multiple glacial phases
DOI: 10.1130/G24382A.1 Bibcode: 2008Geo....36..411D

Head, James W.; Marchant, David R.; Dickson, James L.

Lineated valley fill (LVF) in fretted valleys at the dichotomyboundary has been interpreted as glacial in origin. Unknownare (1) the original thickness of the glacier ice, (2) the amountof ice-surface lowering, through sublimation and retreat, toits presently observed level, and (3) whether there were multipleperiods of glaciation. We address thes…

2008 Geology
MEx 108
The E ring in the vicinity of Enceladus. I. Spatial distribution and properties of the ring particles
DOI: 10.1016/j.icarus.2007.06.027 Bibcode: 2008Icar..193..420K

Beckmann, U.; Kempf, S.; Postberg, F. +6 more

Saturn's diffuse E ring is the largest ring of the Solar System and extends from about 3.1R (Saturn radius R=60,330 km) to at least 8R encompassing the icy moons Mimas, Enceladus, Tethys, Dione, and Rhea. After Cassini's insertion into her saturnian orbit in July 2004, the spacecraft performed a number of equatorial as well as steep traversals thr…

2008 Icarus
Cassini 107
Effects of Dust Geometry in Lyα Galaxies at z = 4.4
DOI: 10.1086/525272 Bibcode: 2008ApJ...678..655F

Finkelstein, Steven L.; Malhotra, Sangeeta; Grogin, Norman +2 more

Equivalent widths (EWs) observed in high-redshift Lyα galaxies could be stronger than the EW intrinsic to the stellar population if dust is present residing in clumps in the interstellar medium (ISM). In this scenario, continuum photons could be extinguished, while the Lyα photons would be resonantly scattered by the clumps, eventually escaping th…

2008 The Astrophysical Journal
eHST 107
On the kinematic evolution of young local associations and the Scorpius-Centaurus complex
DOI: 10.1051/0004-6361:20077720 Bibcode: 2008A&A...480..735F

Figueras, F.; Torra, J.; Fernández, D.

Context: Over the last decade, several groups of young (mainly low-mass) stars have been discovered in the solar neighbourhood (closer than ~100 pc), thanks to cross-correlation between X-ray, optical spectroscopy and kinematic data. These young local associations - including an important fraction whose members are Hipparcos stars - offer insights…

2008 Astronomy and Astrophysics
Hipparcos 107
Metal-rich multi-phase gas in M 87. AGN-driven metal transport, magnetic-field supported multi-temperature gas, and constraints on non-thermal emission observed with XMM-Newton
DOI: 10.1051/0004-6361:20078749 Bibcode: 2008A&A...482...97S

Finoguenov, A.; Böhringer, H.; Simionescu, A. +2 more

We use deep (~120 ks) XMM-Newton data of the M 87 halo to analyze its spatially resolved temperature structure and chemical composition. We focus particularly on the regions of enhanced X-ray brightness associated with the inner radio lobes, which are known not to be described very well by single-temperature spectral models. Compared to a simple t…

2008 Astronomy and Astrophysics
XMM-Newton 106
New observations of the extended hydrogen exosphere of the extrasolar planet HD 209458b
DOI: 10.1051/0004-6361:200809460 Bibcode: 2008A&A...483..933E

Ehrenreich, D.; Ferlet, R.; Vidal-Madjar, A. +6 more

Context: Atomic hydrogen escaping from the planet HD 209458b provides the largest observational signature ever detected for an extrasolar planet atmosphere. However, the Space Telescope Imaging Spectrograph (STIS) used in previous observational studies is no longer available, whereas additional observations are still needed to b…

2008 Astronomy and Astrophysics
eHST 106
High Metallicity of the X-Ray Gas Up to the Virial Radius of a Binary Cluster of Galaxies: Evidence of Galactic Superwinds at High-Redshift
DOI: 10.1093/pasj/60.sp1.S343 Bibcode: 2008PASJ...60S.343F

Reiprich, Thomas H.; Hayashida, Kiyoshi; Matsumoto, Hironori +4 more

We present an analysis of a Suzaku observation of the link region between the galaxy clusters A 399 and A 401. We obtained the metallicity of the intracluster medium (ICM) up to the cluster virial radii for the first time. We determined the metallicity where the virial radii of the two clusters cross each other (∼2 Mpc away from their centers) and…

2008 Publications of the Astronomical Society of Japan
Suzaku 106
Water vapour jets inside the plume of gas leaving Enceladus
DOI: 10.1038/nature07542 Bibcode: 2008Natur.456..477H

Hansen, C. J.; Hendrix, A. R.; Colwell, J. E. +7 more

A plume of water vapour escapes from fissures crossing the south polar region of the Saturnian moon Enceladus. Tidal deformation of a thin surface crust above an internal ocean could result in tensile and compressive stresses that would affect the width of the fissures; therefore, the quantity of water vapour released at different locations in Enc…

2008 Nature
Cassini 106