Search Publications

Rotational dynamics of subsolar sublimating triaxial comets
DOI: 10.1016/j.pss.2004.04.001 Bibcode: 2004P&SS...52..897M

Mysen, Eirik

A model with subsolar water sublimation on a triaxial, ellipsoidal comet nucleus is presented for the calculation of reactive torques. The resulting differential equations describing the comet's rotation are then Hamiltonian, and gravity-gradients are trivial to include. While effects derived from a weak perturbing function are neither able to cha…

2004 Planetary and Space Science
Rosetta 10
The discovery of hard X-ray emission in the persistent flux of the Rapid Burster
DOI: 10.1051/0004-6361:20041243 Bibcode: 2004A&A...426..979F

Frontera, F.; Goldoni, P.; Stella, L. +3 more

We report the first detection with INTEGRAL of persistent hard X-ray emission (20 to 100 keV) from the Rapid Burster (MXB 1730-335), and describe its full spectrum from 3 to 100 keV. The source was detected on February/March 2003 during one of its recurrent outbursts. The source was clearly detected with a high signal to noise ratio during the sin…

2004 Astronomy and Astrophysics
INTEGRAL 10
Hα kinematics of a z~ 1 disc galaxy from near-infrared integral field spectroscopy
DOI: 10.1111/j.1365-2966.2004.08323.x Bibcode: 2004MNRAS.354L..19S

Aragón-Salamanca, A.; Swinbank, A. M.; Abraham, R. G. +6 more

In this Letter we present the first 3D spectroscopic study of Hα emission in a z~ 1 field galaxy with an integral field unit. Using the Cambridge Infrared Panoramic Survey Spectrograph (CIRPASS) on Gemini-South, we map the spatial and velocity distribution of Hα emission in the z= 0.819 galaxy CFRS 22.1313. We detect two Hα emitting regions with a…

2004 Monthly Notices of the Royal Astronomical Society
eHST 10
The X-ray halo of G21.5 - 0.9
DOI: 10.1016/j.asr.2003.04.025 Bibcode: 2004AdSpR..33..398B

Bocchino, F.; Bandiera, R.

The emission of the plerion G21.5 - 0.9 appears more extended in X-rays than in radio. This is an unexpected result because it would imply that short-lived X-ray electrons may reach distances even larger than radio electrons. Applying an empirical relationship between dust scattering optical depth and photoelectric column density, the measured col…

2004 Advances in Space Research
XMM-Newton 10
High frequency ion sound waves associated with Langmuir waves in type III radio burst source regions
DOI: 10.5194/npg-11-411-2004 Bibcode: 2004NPGeo..11..411T

MacDowall, R. J.; Thejappa, G.

Short wavelength ion sound waves (2-4kHz) are detected in association with the Langmuir waves (~15-30kHz) in the source regions of several local type III radio bursts. They are most probably not due to any resonant wave-wave interactions such as the electrostatic decay instability because their wavelengths are much shorter than those of Langmuir w…

2004 Nonlinear Processes in Geophysics
Ulysses 10
A study of the electrical charging of the Rosetta orbiter: 2. Experimental tests in a laboratory plasma
DOI: 10.1029/2003JA009834 Bibcode: 2004JGRA..109.1105B

Berthelier, Jean-Jacques; Roussel, Jean-FrançOis

Following the numerical simulation presented in the companion paper, we have performed experimental tests in a plasma simulation chamber to check the results of the numerical model and validate its capability to properly predict the electrical equilibrium of the Rosetta orbiter. Since low temperature cometary plasmas cannot be directly reproduced …

2004 Journal of Geophysical Research (Space Physics)
Rosetta 10
Physical parameters of helium-rich subdwarf B stars from spectral energy distributions
DOI: 10.1051/0004-6361:20031577 Bibcode: 2004A&A...413..323A

Jeffery, C. S.; Ahmad, A.

We present effective temperatures and angular radii for eleven helium-rich subdwarf B stars. These are measured using spectral energy distributions from archival IUE spectra and existing optical and infrared photometry. The data have been analysed using a grid of high-gravity helium-rich LTE model atmospheres and a χ2-minimization proce…

2004 Astronomy and Astrophysics
IUE 10
XMM-Newton surveys of the Canada-France Redshift Survey fields - II. The X-ray catalogues, the properties of the host galaxies and the redshift distribution
DOI: 10.1111/j.1365-2966.2004.07703.x Bibcode: 2004MNRAS.350..785W

Nandra, K.; Lilly, S.; McCracken, H. J. +5 more

We present the X-ray source catalogues for the XMM surveys of the 3-h and 14-h Canada-France Redshift Survey fields (0.5-10 keV flux range ~2 × 10-15-10-13 erg cm-2 s-1). We use a subset of the XMM sources, which have Chandra positions, to determine the best method of obtaining optical identifications of…

2004 Monthly Notices of the Royal Astronomical Society
XMM-Newton 10
Statistical behavior of foreshock Langmuir waves observed by the Cluster wideband data plasma wave receiver
DOI: 10.5194/angeo-22-2337-2004 Bibcode: 2004AnGeo..22.2337S

Balogh, A.; Lucek, E.; Gurnett, D. +3 more

Available from http://www.copernicus.org/site/EGU/annales/22/7/2337.htm?FrameEngine=false;

2004 Annales Geophysicae
Cluster 9
Mafic silicate mapping on Mars: effects of palagonitic material, multiple mafic silicates, and spectral resolution
DOI: 10.1016/j.icarus.2004.06.002 Bibcode: 2004Icar..172..233C

Bell, James F.; Cloutis, Edward A.

The visible to near-infrared spectral reflectance properties of intimate and areal pyroxene + palagonitic material mixtures as well as pure mafic silicates (low-calcium pyroxene, high-calcium pyroxene, pigeonite, olivine) and mixtures of these minerals were analyzed at high spectral resolution (5 nm) as well as with non-contiguous band passes equi…

2004 Icarus
eHST 9