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Multi-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL. II. The environment of the companion star
DOI: 10.1051/0004-6361:20078774 Bibcode: 2008A&A...484..801R

Pantin, E.; Chaty, S.; Rahoui, F. +1 more

Context: The INTEGRAL mission has led to the discovery of a new type of supergiant X-ray binaries (SGXBs), whose physical properties differ from those of previously known SGXBs. Those sources are in the course of being unveiled by means of multi-wavelength X-rays, optical, near- and mid-infrared observations, and two classes are appearing. The fir…

2008 Astronomy and Astrophysics
INTEGRAL 142
Compositional mapping of Saturn's satellite Dione with Cassini VIMS and implications of dark material in the Saturn system
DOI: 10.1016/j.icarus.2007.08.035 Bibcode: 2008Icar..193..372C

Nicholson, Philip D.; Baines, Kevin H.; Buratti, Bonnie J. +9 more

Cassini VIMS has obtained spatially resolved imaging spectroscopy data on numerous satellites of Saturn. A very close fly-by of Dione provided key information for solving the riddle of the origin of the dark material in the Saturn system. The Dione VIMS data show a pattern of bombardment of fine, sub-0.5-µm diameter particles impacting the s…

2008 Icarus
Cassini 142
Constraints on decaying dark matter from XMM-Newton observations of M31
DOI: 10.1111/j.1365-2966.2008.13266.x Bibcode: 2008MNRAS.387.1361B

Boyarsky, Alexey; Ruchayskiy, Oleg; Iakubovskyi, Dmytro +1 more

We derive constraints on the parameters of the radiatively decaying dark matter (DM) particle, using the XMM-Newton EPIC spectra of the Andromeda galaxy (M31). Using the observations of the outer (5-13arcmin) parts of M31, we improve the existing constraints. For the case of sterile neutrino DM, combining our constraints with the latest computatio…

2008 Monthly Notices of the Royal Astronomical Society
XMM-Newton 142
Wavelengths and Intensities of Spectral Lines in the 171-211 and 245-291 Å Ranges from Five Solar Regions Recorded by the Extreme-Ultraviolet Imaging Spectrometer (EIS) on Hinode
DOI: 10.1086/529378 Bibcode: 2008ApJS..176..511B

Brown, C. M.; Hara, H.; Feldman, U. +2 more

We present spectral line wavelengths, identifications, and intensities in the 171-211 and 245-291 Å ranges from five solar plasma regions recorded by the Extreme-Ultraviolet Imaging Spectrometer (EIS) on Hinode. The recorded data were emitted from a quiet region, two active areas on the solar disk, a limb region, and a region 20'' above the limb. …

2008 The Astrophysical Journal Supplement Series
Hinode 142
Polarization of the Crab Pulsar and Nebula as Observed by the INTEGRAL/IBIS Telescope
DOI: 10.1086/593974 Bibcode: 2008ApJ...688L..29F

Grenier, I. A.; Laurent, P.; Lebrun, F. +2 more

Neutron stars generate powerful winds of relativistic particles that form bright synchrotron nebulae around them. Polarimetry provides a unique insight into the geometry and magnetic configuration of the wind, but high-energy measurements have failed until recently. The INTEGRAL/IBIS telescope has been used in its Compton mode to search for linear…

2008 The Astrophysical Journal
INTEGRAL 140
The Spatial Structure of an Accretion Disk
DOI: 10.1086/524190 Bibcode: 2008ApJ...673...34P

Kochanek, Christopher S.; Poindexter, Shawn; Morgan, Nicholas

Based on the microlensing variability of the two-image gravitational lens HE 1104-1805 observed between 0.4 and 8 µm, we have measured the size and wavelength-dependent structure of the quasar accretion disk. Modeled as a power law in temperature, T propto R, we measure a B-band (0.13 µm in the rest frame) half-light radiu…

2008 The Astrophysical Journal
eHST 140
An update to a Saturnian longitude system based on kilometric radio emissions
DOI: 10.1029/2007JA012861 Bibcode: 2008JGRA..113.5222K

Gurnett, D. A.; Kurth, W. S.; Averkamp, T. F. +2 more

The period of Saturn kilometric radiation modulation as determined by Voyager forms the basis for a longitude system (SLS) recognized by the International Astronomical Union. However, Ulysses and Cassini observations have shown that this modulation period varies by the order of one percent on timescales of a few years and, hence, does not represen…

2008 Journal of Geophysical Research (Space Physics)
Cassini Ulysses 139
A systematic look at the very high and low/hard state of GX339-4: constraining the black hole spin with a new reflection model
DOI: 10.1111/j.1365-2966.2008.13358.x Bibcode: 2008MNRAS.387.1489R

Fabian, A. C.; Miller, J. M.; Miniutti, G. +3 more

We present a systematic study of GX 339-4 in both its very high and low hard states from simultaneous observations made with XMM-Newton and RXTE in 2002 and 2004. The X-ray spectra of both these extreme states exhibit strong reflection signatures, with a broad, skewed Fe Kα line clearly visible above the continuum. Using a newly developed, self-co…

2008 Monthly Notices of the Royal Astronomical Society
XMM-Newton 139
Dynamical Centers and Noncircular Motions in THINGS Galaxies: Implications for Dark Matter Halos
DOI: 10.1088/0004-6256/136/6/2720 Bibcode: 2008AJ....136.2720T

Walter, F.; Brinks, E.; de Blok, W. J. G. +2 more

We present harmonic decompositions of the velocity fields of 19 galaxies from The H I Nearby Galaxy Survey (THINGS) which quantify the magnitude of the noncircular motions in these galaxies and yield observational estimates of the elongations of the dark matter halo potentials. Additionally, we present accurate dynamical center positions for these…

2008 The Astronomical Journal
eHST 138
Magnetic Field Overlying Solar Eruption Regions and Kink and Torus Instabilities
DOI: 10.1086/589282 Bibcode: 2008ApJ...679L.151L

Liu, Y.

Using a potential field source surface (PFSS) model, we study a magnetic field overlying erupted filaments in solar active regions. The filaments studied here were reported to experience a kink instability or a torus instability. The torus instability leads to a full eruption, while the kink instability leads to a full eruption or a failed eruptio…

2008 The Astrophysical Journal
SOHO 138