Search Publications

Formation of Saturn's ring spokes by lightning-induced electron beams
DOI: 10.1029/2006GL028146 Bibcode: 2006GeoRL..3321202J

Krupp, N.; Woch, J.; Fränz, M. +10 more

Spokes are near-linear markings sometimes visible on Saturn's rings. They are widely accepted as being electrostatically-levitated sheets of ~0.6 micron-radius charged grains. Previously-suggested causes of the grains' charging do not agree with all spoke characteristics, which include their rapid generation, localized formation primarily in Satur…

2006 Geophysical Research Letters
Cassini 25
The X-ray properties of optically selected z > 0.6 clusters in the European Southern Observatory Distant Cluster Survey
DOI: 10.1111/j.1365-2966.2006.10796.x Bibcode: 2006MNRAS.371.1777J

Pelló, R.; Milvang-Jensen, B.; Halliday, C. +11 more

We present XMM-Newton observations of three optically selected z > 0.6 clusters from the European Southern Observatory (ESO) Distant Cluster Survey (EDisCS), comprising the first results of a planned X-ray survey of the full EDisCS high-redshift sample. The EDisCS clusters were identified in the Las Campanas Distant Cluster Survey as surface br…

2006 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 25
The Influence of Mass and Environment on the Evolution of Early-Type Galaxies
DOI: 10.1086/507582 Bibcode: 2006ApJ...647L..99D

Lanzoni, Barbara; Jørgensen, Inger; di Serego Alighieri, Sperello

We report on a uniform comparative analysis of the fundamental parameters of early-type galaxies at z~1 down to MB<=-20, both in the field and in clusters. The changes in the M/LB ratio from z~1 to today are larger for lower mass galaxies in all environments, and are larger in the field than in clusters for galaxies with t…

2006 The Astrophysical Journal
eHST 25
Lightning detection on the Venus Express mission
DOI: 10.1016/j.pss.2006.04.026 Bibcode: 2006P&SS...54.1344R

Russell, C. T.; Zhang, T. L.; Strangeway, R. J.

Radio waves and optical flashes consistent with the lightning generation have been reported frequently at Venus. These observations point to the presence of electrical discharges in the sulfuric acid clouds of Venus. A particularly strong whistler-mode signal has been found propagating parallel to the magnetic field in the night ionosphere near 10…

2006 Planetary and Space Science
VenusExpress 25
Estimated IR and phosphorescence emission fluxes for specific polycyclic aromatic hydrocarbons in the Red Rectangle
DOI: 10.1051/0004-6361:20053738 Bibcode: 2006A&A...446..537M

Joblin, C.; Toublanc, D.; Mulas, G. +1 more

Following tentative identification of the blue luminescence in the Red Rectangle by Vijh et al., we computed absolute fluxes for the vibrational IR emission and phosphorescence bands of three small polycyclic aromatic hydrocarbons. The calculated IR spectra were compared with available ISO observations. A subset of the emission …

2006 Astronomy and Astrophysics
ISO 25
On the Propagation and Dissipation of Alfvén Waves in Coronal Holes
DOI: 10.1007/s11207-006-0141-2 Bibcode: 2006SoPh..237..143D

Srivastava, A. K.; Dwivedi, B. N.

We underline the importance of Alfvén wave dissipation in the magnetic funnels through the viscous and resistive plasma. Our results show that Alfvén waves are one of the primary energy sources in the innermost part of coronal holes where the solar wind outflow starts.

2006 Solar Physics
SOHO 25
XMM-Newton observations of the complex spin pulse of the intermediate polar PQ Geminorum
DOI: 10.1111/j.1365-2966.2006.10368.x Bibcode: 2006MNRAS.369.1229E

Hellier, Coel; Ramsay, Gavin; Evans, P. A.

The intermediate polar PQ Geminorum shows a complex pulsation, caused by a spinning white dwarf, which varies markedly with wavelength. We report XMM-Newton observations, including the soft and hard X-ray bands and the first ultraviolet light curves of this star. We update the ephemeris for PQ Gem allowing us to align these data with a compilation…

2006 Monthly Notices of the Royal Astronomical Society
XMM-Newton 25
Improved input to the empirical coronal mass ejection (CME) driven shock arrival model from CME cone models
DOI: 10.1029/2006SW000227 Bibcode: 2006SpWea...410002X

St. Cyr, O. C.; Gopalswamy, N.; Michalek, G. +4 more

We study the Sun-Earth travel time of interplanetary shocks driven by coronal mass ejections (CMEs) using empirical cone models. Three different cone models have been used to obtain the radial speeds of the CMEs, which are then used as input to the empirical shock arrival (ESA) model to obtain the Sun to Earth travel time of the shocks. We compare…

2006 Space Weather
SOHO 25
Understanding the Nuclear Gas Dispersion in Early-Type Galaxies in the Context of Black Hole Demographics
DOI: 10.1086/500973 Bibcode: 2006AJ....131.1961V

van der Marel, Roeland P.; Verdoes Kleijn, Gijs A.; Noel-Storr, Jacob

The majority of nearby early-type galaxies contain detectable amounts of emission-line gas at their centers. The nuclear gas kinematics form a valuable diagnostic of the central black hole (BH) mass. Here we analyze and model Hubble Space Telescope STIS observations of a sample of 27 galaxies; 16 Fanaroff-Riley Type I radio galaxies and 11 (more) …

2006 The Astronomical Journal
eHST 25
A model of the ionosphere of Saturn's rings and its implications
DOI: 10.1016/j.icarus.2005.11.022 Bibcode: 2006Icar..181..465L

Luhmann, J. G.; Tokar, R. L.; Johnson, R. E. +2 more

The detection of cold O2+ and O + ions in the vicinity of Saturn's rings during the Cassini Orbiter orbit insertion confirmed expectations that the rings would have a water product atmosphere and ionosphere. These observations prompted a new look at their origin and nature by Johnson et al. [Johnson, R.E., Luhmann, J.G., Tokar, R.L., Bo…

2006 Icarus
Cassini 25