Search Publications

Three-dimensional finite difference time domain modeling of the Schumann resonance parameters on Titan, Venus, and Mars
DOI: 10.1029/2005RS003431 Bibcode: 2006RaSc...41.2S03Y

Yang, Heng; Pasko, Victor P.; Yair, Yoav

The conducting ionosphere and conducting surface of Titan, Venus, and Mars form a concentric resonator, which would support the possibility of the existence of global electromagnetic resonances. On Earth, such resonances are commonly referred to as Schumann resonances and are excited by lightning discharges. The detection of such resonances on oth…

2006 Radio Science
Cassini 33
Disentangling the synchrotron and inverse Compton variability in the X-ray emission of the intermediate BL Lacertae object S5 0716+71
DOI: 10.1051/0004-6361:20065317 Bibcode: 2006A&A...457..133F

Emmanoulopoulos, D.; Wagner, S. J.; Ferrero, E. +1 more

Context: .The possibility to detect simultaneously in the X-ray band the synchrotron and Inverse Compton (IC) emission of intermediate BL Lac objects offers the unique opportunity to study contemporaneously the low- and high-energy tails of the electron distribution in the jets of these sources.
Aims: .We attempted to disentangle the X-ray spe…

2006 Astronomy and Astrophysics
XMM-Newton 33
The Rate of Emergence of Magnetic Dipoles in Coronal Holes and Adjacent Quiet-Sun Regions
DOI: 10.1086/503870 Bibcode: 2006ApJ...641L..65A

Abramenko, V. I.; Yurchyshyn, V. B.; Fisk, L. A.

Observations from the Michelson Doppler Imager and the EUV Imaging Telescope on the Solar and Heliospheric Observatory are analyzed to determine the rate of emergence of new magnetic flux in coronal holes and in surrounding regions on the quiet Sun. Coronal holes are regions where the open magnetic flux of the Sun, the component that forms the hel…

2006 The Astrophysical Journal
SOHO 33
An XMM-Newton view of the young open cluster NGC 6231. I. The catalogue
DOI: 10.1051/0004-6361:20053224 Bibcode: 2006A&A...454.1047S

Gosset, E.; Rauw, G.; Vreux, J. -M. +2 more

This paper is the first of a series dedicated to the X-ray properties of the young open cluster NGC 6231. Our data set relies on an XMM-Newton campaign of a nominal duration of 180 ks and reveals that NGC 6231 is very rich in the X-ray domain too. Indeed, 610 X-ray sources are detected in the present field of view, centered on the cluster core. Th…

2006 Astronomy and Astrophysics
XMM-Newton 33
Cluster survey of the mid-altitude cusp: 1. size, location, and dynamics
DOI: 10.5194/angeo-24-3011-2006 Bibcode: 2006AnGeo..24.3011P

Escoubet, C. P.; Pitout, F.; Klecker, B. +1 more

We present a statistical study of four years of Cluster crossings of the mid-altitude cusp. In this first part of the study, we start by introducing the method we have used a) to define the cusp properties, b) to sort the interplanetary magnetic field (IMF) conditions or behaviors into classes, c) to determine the proper time delay between the sol…

2006 Annales Geophysicae
Cluster 33
The DEEP Groth Strip Survey. VI. Spectroscopic, Variability, and X-Ray Detection of Active Galactic Nuclei
DOI: 10.1086/505909 Bibcode: 2006ApJS..166...69S

Kobulnicky, Henry A.; Gebhardt, Karl; Willmer, Christopher N. A. +8 more

We identify active galactic nuclei (AGNs) in the Groth-Westphal Survey Strip (GSS) using the independent and complementary selection techniques of optical spectroscopy and photometric variability. We discuss the X-ray properties of these AGNs using Chandra/XMM-Newton data for this region. From a sample of 576 galaxies with high-quality spectra we …

2006 The Astrophysical Journal Supplement Series
eHST 33
Saturn's auroral morphology and activity during quiet magnetospheric conditions
DOI: 10.1029/2006JA011965 Bibcode: 2006JGRA..11112210G

Coates, A. J.; Dougherty, M. K.; Kurth, W. S. +8 more

We report the results of a coordinated Hubble Space Telescope-Cassini campaign that took place between 26 October and 2 November 2005. During this period, Saturn's magnetosphere was in an expanded state and the solar wind was quiet, as indicated by the location of the magnetopause, in situ particle measurements, weak auroral SKR emission, and the …

2006 Journal of Geophysical Research (Space Physics)
Cassini eHST 33
Analysis and Interpretation of Hard X-Ray Emission from the Bullet Cluster (1ES 0657-558), the Most Distant Cluster of Galaxies Observed by RXTE
DOI: 10.1086/508564 Bibcode: 2006ApJ...652..948P

Madejski, Greg; Petrosian, Vahé; Luli, Kevin

Evidence for nonthermal activity in clusters of galaxies is well established from radio observations of synchrotron emission by relativistic electrons. New windows in the extreme-ultraviolet and hard X-ray ranges have provided more powerful tools for the investigation of this phenomenon. Detections of hard X-rays in the 20-100 keV range have been …

2006 The Astrophysical Journal
XMM-Newton 33
A Spitzer IRAC Search for Substellar Companions of the Debris Disk Star ɛ Eridani
DOI: 10.1086/505531 Bibcode: 2006ApJ...647.1437M

Stapelfeldt, K. R.; Fazio, G. G.; Marengo, M. +3 more

We have used the Infrared Array Camera (IRAC) on board the Spitzer Space Telescope to search for low-mass companions of the nearby debris disk star ɛ Eri. The star was observed in two epochs 39 days apart, with different focal plane rotation to allow the subtraction of the instrumental point-spread function, achieving a maximum sensitivity of 0.01…

2006 The Astrophysical Journal
eHST 33
Structural parameters from ground-based observations of newly discovered globular clusters in NGC 5128
DOI: 10.1051/0004-6361:20053393 Bibcode: 2006A&A...447..877G

Geisler, D.; Gómez, M.; Richtler, T. +3 more

We have investigated a number of globular cluster candidates from a recent wide-field study by Harris et al. (2004a, AJ, 128, 712) of the giant elliptical galaxy NGC 5128. We used the Magellan I telescope + MagIC camera under excellent seeing conditions (0.3 arcsec-0.6 arcsec) and obtained very high resolution images for a sampl…

2006 Astronomy and Astrophysics
eHST 33