Search Publications

037-B327 in M31: Luminous Globular Cluster or Core of a Former Dwarf Spheroidal Companion to M31?
DOI: 10.1086/500257 Bibcode: 2006ApJ...636L..93M

Zhou, Xu; van den Bergh, Sidney; Ma, Jun +6 more

The cluster 037-B327 is of interest because it is both the most luminous and the most highly reddened cluster known in M31. Deep observations with the Advanced Camera for Surveys on the Hubble Space Telescope provide photometric data in the F606W band and also show that this cluster is crossed by a dust lane. We have determined the structural para…

2006 The Astrophysical Journal
eHST 20
Hipparcos astrometric orbits for two brown dwarf companions: HD 38529 and HD 168443
DOI: 10.1051/0004-6361:20054611 Bibcode: 2006A&A...449..699R

Quirrenbach, A.; Reffert, S.

Context: .HD 38529 and HD 168443 have previously been identified as systems with two substellar companion candidates using precise radial velocity measurements.Aims.We want to further constrain their orbits and the nature of the outer companions.Methods.We fit astrometric orbits of the outer substellar companions in the two systems to the Hipparco…

2006 Astronomy and Astrophysics
Hipparcos 20
Optical/near-infrared observations of the black hole candidate XTE J1720-318 : from high-soft to low-hard state
DOI: 10.1051/0004-6361:20054735 Bibcode: 2006A&A...455..639C

Chaty, S.; Bessolaz, N.

Aims.To gain a better understanding of high-energy Galactic sources, we observed the Galactic X-ray binary and black hole candidate XTE J1720-318 in the optical and near-infrared, just after the onset of its X-ray outburst in January, 2003. These observations were obtained with the ESO/NTT as the Target of Opportunity, in February and April 2003.<…

2006 Astronomy and Astrophysics
INTEGRAL 20
Multiplet structure of acceleration processes in the distant magnetotail
DOI: 10.1029/2005GL024901 Bibcode: 2006GeoRL..33.6105Z

Zelenyi, L. M.; Sauvaud, J. -A.; Grigorenko, E. E. +1 more

We have studied ion distributions measured in the Plasma Sheet Boundary Layer (PSBL) of the Earth's magnetotail by the Cluster spacecraft at X ~ -15Re. Field-aligned ion beams (beamlets) accelerated in the magnetotail to energies of ~30keV are typically observed within the interface region between the Plasma Sheet (PS) and the magnetotail lobes. P…

2006 Geophysical Research Letters
Cluster 20
The Frequency of Binary Kuiper Belt Objects
DOI: 10.1086/504940 Bibcode: 2006ApJ...643L..57K

Elliot, J. L.; Kern, S. D.

We estimate the frequency of widely spaced (separations greater than 0.5") Kuiper Belt binaries (KBBs) from surveys for new Kuiper Belt objects (KBOs) with the Deep Ecliptic Survey and through recovery observations for newly discovered KBOs at the Magellan telescopes. We find the frequency of KBBs versus discovery separation to be related by an in…

2006 The Astrophysical Journal
eHST 20
The intensity contrast of solar photospheric faculae and network elements. II. Evolution over the rising phase of solar cycle 23
DOI: 10.1051/0004-6361:20053869 Bibcode: 2006A&A...452..311O

Sanahuja, B.; Ortiz, A.; Domingo, V.

We studied the radiative properties of small magnetic elements (active region faculae and the network) during the rising phase of solar cycle 23 from 1996 to 2001, determining their contrasts as a function of heliocentric angle, magnetogram signal, and the solar cycle phase. We combined near-simultaneous full disk images of the line-of-sight magne…

2006 Astronomy and Astrophysics
SOHO 20
Cassini observations of the Interplanetary Medium Upstream of Saturn and their relation to the Hubble Space Telescope aurora data
DOI: 10.1016/j.asr.2005.08.005 Bibcode: 2006AdSpR..38..806B

Dougherty, M. K.; Jackman, C. M.; Clarke, J. T. +3 more

We present Cassini magnetometer and plasma data for the January 2004 ‘solar wind campaign’ in which the particles and fields instruments monitored the solar wind and interplanetary magnetic field, while the Hubble Space Telescope (HST) simultaneously observed the UV aurora in Saturn’s southern ionosphere. Clear structuring is evident in the data w…

2006 Advances in Space Research
Cassini eHST 20
Small-Scale Anisotropy and Intermittence in High- and Low-Latitude Solar Wind
DOI: 10.1086/498665 Bibcode: 2006ApJ...638..499B

Velli, M.; Biferale, L.; Bigazzi, A. +1 more

We study low- and high-latitude fast solar wind data from the Ulysses spacecraft from 1992 to 1994 using for the first time a systematic method to analyze the anisotropic content of the magnetic field fluctuations beyond second-order correlation functions. We investigate all available frequencies, 1-10-6 Hz, for both high- and low-latit…

2006 The Astrophysical Journal
Ulysses 20
Comet 67P/Churyumov Gerasimenko: Modeling of orientation and structure
DOI: 10.1016/j.pss.2005.09.001 Bibcode: 2006P&SS...54...15K

Kossacki, Konrad J.; Szutowicz, Sławomira

The comet 67P/Churyumov-Gerasimenko is the current target of the mission Rosetta, initially planned to investigate comet 46P/Wirtanen. These two comets have similar orbits, except the distance to the Sun at perihelion, but different orbital histories and different masses. Thus, structures of the nuclei can be significantly different. The evolution…

2006 Planetary and Space Science
Rosetta 20
Source location of the wedge-like dispersed ring current in the morning sector during a substorm
DOI: 10.1029/2006JA011621 Bibcode: 2006JGRA..11111S09Y

Lundin, R.; Yamauchi, M.; Balogh, A. +8 more

Source of wedge-like dispersed sub-keV ring current ions (wedge-like structure) is investigated using Cluster CIS data. Statistics from nearly 550 traversals show that the wedge-like structure with upper energy extending to ordinary energy of ring current is found mostly in the morning sector whereas those limited within sub-keV range are found mo…

2006 Journal of Geophysical Research (Space Physics)
Cluster 20