Search Publications

Astrometry of Saturn's Satellites from the Hubble Space Telescope WFPC2
DOI: 10.1086/499215 Bibcode: 2006PASP..118..246F

French, R. G.; Verbiscer, A.; McGhee, C. A. +4 more

Highly accurate astrometric positions of 14 of Saturn's satellites have been obtained from 444 Hubble Space Telescope images taken with the Wide Field Planetary Camera 2 (WFPC2) between 1996 and 2005. In all, 1036 satellite positions were measured in Planetary Camera (PC) frames, with a typical uncertainty of σPC=0.014" (80 km at Saturn…

2006 Publications of the Astronomical Society of the Pacific
eHST 17
Cluster satellite observations of mHz pulsations in the dayside magnetosphere
DOI: 10.1016/j.asr.2005.04.103 Bibcode: 2006AdSpR..38.1730E

Glassmeier, K. -H.; Blomberg, L. G.; Eriksson, P. T. I.

On 17 August 2002 the Cluster spacecraft moved through the dayside magnetosphere. Between 16:00 and 18:30 UT clear monochromatic oscillations are seen in both electric field and magnetometer data. The frequency is 4.2 mHz in the spacecraft frame of reference. The oscillations have a clear spatial localisation. The magnetic field oscillations are r…

2006 Advances in Space Research
Cluster 17
Observational evidence for AGN fueling: I. The case of NGC 6104â€''Merging with a companion
DOI: 10.1134/S1063773706080032 Bibcode: 2006AstL...32..520S

Moiseev, A. V.; Afanasiev, V. L.; Smirnova, A. A.

We investigate in detail the kinematics and morphology of the Seyfert galaxy NGC 6104 in order to identify the mechanism of gas transportation to the active galactic nucleus (AGN). Our observational data were obtained at the 6-m Special Astrophysical Observatory telescope with the MPFS integral-field spectrograph and the SCORPIO universal device i…

2006 Astronomy Letters
eHST 17
Energetic nitrogen ions within the inner magnetosphere of Saturn
DOI: 10.1029/2004JA010509 Bibcode: 2006JGRA..111.9223S

Johnson, R. E.; Paranicas, C.; Sittler, E. C. +9 more

We investigate the importance of nitrogen ions within Saturn's magnetosphere and their contribution to the energetic charged particle population within Saturn's inner magnetosphere. This study is based on the Voyager observations of Saturn's magnetosphere and Cassini observations. The latter have shown that water group ions dominate both the plasm…

2006 Journal of Geophysical Research (Space Physics)
Cassini 17
Three Gravitational Lenses for the Price of One: Enhanced Strong Lensing through Galaxy Clustering
DOI: 10.1086/507623 Bibcode: 2006ApJ...651..667F

McKean, J. P.; Treu, T.; Blandford, R. D. +7 more

We report the serendipitous discovery of two strong gravitational lens candidates (ACS J160919+6532 and ACS J160910+6532) in deep images obtained with the Advanced Camera for Surveys on the Hubble Space Telescope, each less than 40" from the previously known gravitational lens system CLASS B1608+656. The redshifts of both lens galaxies have been m…

2006 The Astrophysical Journal
eHST 17
Energy-dispersed ions in the plasma sheet boundary layer and associated phenomena: Ion heating, electron acceleration, Alfvén waves, broadband waves, perpendicular electric field spikes, and auroral emissions
DOI: 10.5194/angeo-24-2685-2006 Bibcode: 2006AnGeo..24.2685K

Dandouras, I.; Lucek, E.; Fazakerley, A. N. +8 more

Recent Cluster studies reported properties of multiple energy-dispersed ion structures in the plasma sheet boundary layer (PSBL) that showed substructure with several well separated ion beamlets, covering energies from 3 keV up to 100 keV (Keiling et al., 2004a, b). Here we report observations from two PSBL crossings, which show a number of identi…

2006 Annales Geophysicae
Cluster 17
The ZZ Ceti star G 185-32: new insight from asteroseismology
DOI: 10.1051/0004-6361:20054370 Bibcode: 2006A&A...453..219P

Pech, D.; Vauclair, G.

One of the brightest pulsating DA white dwarfs (ZZ Ceti stars), G 185-32, shows 19 periods in its power spectrum, from 71 s to 651 s. Its short periods are among the shortest ones observed in a ZZ Ceti star. The one at 141.9 s shows an amplitude which does not vary with wavelength, in contrast with what the linear theory predicts for ℓ=1 or ℓ=2 no…

2006 Astronomy and Astrophysics
eHST 17
A short introduction to broad and variable iron lines around black holes
DOI: 10.1002/asna.200610669 Bibcode: 2006AN....327..943F

Fabian, A. C.

Accreting black holes often show iron line emission in their X-ray spectra. When this line emission is very broad or variable then it is likely to originate from close to the black hole. The theory and observations of such broad and variable iron lines are briefly reviewed here. In order for a clear broad line to be found, one or more of the follo…

2006 Astronomische Nachrichten
Suzaku 17
CLUSTER observation of collisionless transport at the magnetopause
DOI: 10.1029/2006GL026556 Bibcode: 2006GeoRL..3315109P

Fränz, M.; Dandouras, I.; Rème, H. +5 more

On May 10, 2002 the CLUSTER spacecraft (SC) encountered a ~450 km (five magnetosheath thermal proton gyro-radii) wide high-latitude magnetopause (MP). Magnetic field observations indicate the crossing of a ~130 km thick MP current sheet (CS) located inside a magnetic hole. Proton flux measurements diagnose a dense boundary layer (BL) directly atta…

2006 Geophysical Research Letters
Cluster 17
Three-dimensional Structure of the 2002 April 21 Coronal Mass Ejection
DOI: 10.1086/506981 Bibcode: 2006ApJ...651..566L

Raymond, J. C.; Ko, Y. -K.; Lee, J. -Y. +1 more

A three-dimensional reconstruction of the 2002 April 21 partial halo Coronal Mass Ejection (CME) has been made based on the O VI 1032 Å and [Fe XVIII] 974 Å lines observed by the Ultraviolet Coronagraph Spectrometer (UVCS) on board the Solar and Heliospheric Observatory (SOHO). We use the Doppler velocities to derive the CME structure along the li…

2006 The Astrophysical Journal
SOHO 17