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Electron conductivity and density profiles derived from the mutual impedance probe measurements performed during the descent of Huygens through the atmosphere of Titan
DOI: 10.1016/j.pss.2007.04.008 Bibcode: 2007P&SS...55.1964H

Berthelier, J. J.; Rodrigo, R.; López-Moreno, J. J. +15 more

During the descent of the Huygens probe through the atmosphere of Titan, on January 14th, 2005, the permittivity, waves and altimetry (PWA) subsystem, a component of the Huygens atmospheric structure instrument (HASI), detected an ionized layer at altitudes around 63 km with two different instruments, the relaxation probe (RP) and the mutual imped…

2007 Planetary and Space Science
Huygens 51
A quantitative link between globular clusters and the stellar haloes in elliptical galaxies
DOI: 10.1111/j.1365-2966.2007.12515.x Bibcode: 2007MNRAS.382.1947F

Forte, Juan C.; Faifer, Favio; Geisler, Doug

This paper explores the quantitative connection between globular clusters and the 'diffuse' stellar population of the galaxies they are associated with. Both NGC 1399 and NGC 4486 (M87) are well suited for this kind of analysis due to their large globular cluster populations.

2007 Monthly Notices of the Royal Astronomical Society
eHST 51
Hubble Space Telescope Space Telescope Imaging Spectrograph Spectroscopy of the Environment in the Starburst Core of M82
DOI: 10.1086/522693 Bibcode: 2007ApJ...671..358W

O'Connell, R. W.; Smith, L. J.; Gallagher, J. S., III +3 more

We present optical HST STIS observations made with two slits crossing four of the optically brightest starburst clumps near the nucleus of M82. These provide Hα kinematics, extinction, electron density, and emission measures. From the radial velocity curves derived from both slits we confirm the presence of a stellar bar. We derive a new model for…

2007 The Astrophysical Journal
eHST 51
Mass of Saturn's magnetodisc: Cassini observations
DOI: 10.1029/2006GL028921 Bibcode: 2007GeoRL..34.9108A

André, N.; Coates, A. J.; Russell, C. T. +5 more

Saturn's ring current was observed by Pioneer 11 and the two Voyager spacecraft to extend 8-16 R S in the equatorial plane and appeared to be driven by stress balance with the centrifugal force. We present Cassini observations that show thin current sheets on the dawn flank of Saturn's magnetosphere, symptomatic of the formation of a …

2007 Geophysical Research Letters
Cassini 51
Dynamics of the Narrow-Line Region in the Seyfert 2 Galaxy NGC 1068
DOI: 10.1086/510580 Bibcode: 2007ApJ...656..699D

Kraemer, S. B.; Crenshaw, D. M.; Das, V.

We present dynamical models based on a study of high-resolution long-slit spectra of the narrow-line region (NLR) in NGC 1068 obtained with the Space Telescope Imaging Spectrograph (STIS) aboard the Hubble Space Telescope (HST). The dynamical models consider the radiative force due to the active galactic nucleus (AGN), gravitational forces from th…

2007 The Astrophysical Journal
eHST 51
Nonlinear force-free models for the solar corona. I. Two active regions with very different structure
DOI: 10.1051/0004-6361:20077318 Bibcode: 2007A&A...468..701R

Régnier, S.; Priest, E. R.

Context: With the development of new instrumentation providing measurements of solar photospheric vector magnetic fields, we need to develop our understanding of the effects of current density on coronal magnetic field configurations.
Aims: The object is to understand the diverse and complex nature of coronal magnetic fields in active regions …

2007 Astronomy and Astrophysics
SOHO 51
Evidence that Synchrotron Emission from Nonthermal Electrons Produces the Increasing Submillimeter Spectral Component in Solar Flares
DOI: 10.1007/s11207-007-9044-0 Bibcode: 2007SoPh..245..311S

Costa, J. E. R.; Silva, Adriana V. R.; Kaufmann, P. +4 more

We investigate the origin of the increasing spectra observed at submillimeter wavelengths detected in the flare on 2 November 2003 starting at 17:17 UT. This flare, classified as an X8.3 and 2B event, was simultaneously detected by RHESSI and the Solar Submillimeter Telescope (SST) at 212 and 405 GHz. Comparison of the time profiles at various wav…

2007 Solar Physics
SOHO 51
Chandra and Hubble Space Telescope Observations of Gamma-Ray Blazars: Comparing Jet Emission at Small and Large Scales
DOI: 10.1086/518085 Bibcode: 2007ApJ...662..900T

Maraschi, L.; Wolter, A.; Cheung, C. C. +3 more

We present new Chandra and HST data for four gamma-ray blazars selected on the basis of radio morphology with the aim of revealing X-ray and optical emission from their jets at large scales. All the sources have been detected. Spectral energy distributions (SEDs) of the large-scale jets are obtained as well as new X-ray spectra for the blazar core…

2007 The Astrophysical Journal
eHST 51
GRO J1655-40: Early Stages of the 2005 Outburst
DOI: 10.1086/509755 Bibcode: 2007ApJ...655..434S

Smith, D. A.; Shrader, C. R.; Rupen, M. +4 more

The black hole X-ray binary transient GRO J1655-40 underwent an outburst beginning in early 2005. We present the results of our multiwavelength observational campaign to study the early outburst spectral and temporal evolution, which combines data from X-ray (RXTE and INTEGRAL), radio (VLA), and optical (ROTSE and SMARTS) instruments. During the r…

2007 The Astrophysical Journal
INTEGRAL 51
Orientations of LASCO Halo CMEs and their connection to the flux rope structure of interplanetary CMEs
DOI: 10.1016/j.asr.2007.01.059 Bibcode: 2007AdSpR..40.1821Y

Yurchyshyn, V.; Lynch, B. J.; Lepping, R. P. +2 more

Coronal mass ejections (CMEs) observed near the Sun via LASCO coronographic imaging are the most important solar drivers of geomagnetic storms. ICMEs, their interplanetary, near-Earth counterparts, can be detected in situ, for example, by the Wind and ACE spacecraft. An ICME usually exhibits a complex structure that very often includes a magnetic …

2007 Advances in Space Research
SOHO 50