Search Publications

Experimental study of nonlinear interaction of plasma flow with charged thin current sheets: 1. Boundary structure and motion
DOI: 10.5194/npg-13-365-2006 Bibcode: 2006NPGeo..13..365A

André, M.; Khotyaintsev, Y.; Rème, H. +13 more

We study plasma transport at a thin magnetopause (MP), described hereafter as a thin current sheet (TCS), observed by Cluster at the southern cusp on 13 February 2001 around 20:01 UT. The Cluster observations generally agree with the predictions of the Gas Dynamic Convection Field (GDCF) model in the magnetosheath (MSH) up to the MSH boundary laye…

2006 Nonlinear Processes in Geophysics
Cluster 10
A High-Resolution Spectral Atlas of α Persei from 3810 to 8100 Å
DOI: 10.1086/501231 Bibcode: 2006PASP..118..636L

Galazutdinov, G. A.; Lee, Byeong-Cheol; Park, Myeong-Gu +5 more

We present a high-resolution (λ/δλ=90,000) spectral atlas of the F5 Ib star α Per covering the 3810-8100 Å region. The atlas, based on data obtained with the aid of the echelle spectrograph BOES fed by the 1.8 m telescope at Bohyunsan Observatory (Korea), is the result of the co-addition of a few well-exposed spectra. The final signal-to-noise rat…

2006 Publications of the Astronomical Society of the Pacific
IUE 10
Ultra-luminous sources in nearby galaxies
DOI: 10.1016/j.asr.2006.08.005 Bibcode: 2006AdSpR..38.2793M

Mushotzky, Richard

This paper presents an update of what we have learned in the last year about the ULX phenomenon. New results are presented on radio emission from Holmberg II and a review is given on the recent X-ray data on timing and spectra. The new X-ray spectroscopic and optical imaging survey of nearby ULX with XMM allows us, for the first time, to place the…

2006 Advances in Space Research
XMM-Newton 9
Determination of the microbial diversity of spacecraft assembly, testing and launch facilities: First results of the ESA project MiDiv
DOI: 10.1016/j.asr.2006.01.006 Bibcode: 2006AdSpR..38.1260R

Rettberg, P.; Fritze, D.; Verbarg, S. +4 more

In the near future, an increasing number of in situ life detection and sample return missions to planets and other solar system bodies will be launched. The demand to control spacecraft-carried microbial contamination becomes obvious. COSPAR (Committee of Space Research) has defined guidelines and bioburden limits for different types of missions a…

2006 Advances in Space Research
SMART-1 9
Line formation regions of the UV spectrum of CI Cygni
DOI: 10.1051/0004-6361:20052655 Bibcode: 2006A&A...460..191M

Friedjung, M.; Mikołajewska, J.; Quiroga, C.

Aims.They are the interpretation of the emission line formation regions in CI Cygni
Methods: .They involve the examination of radial velocities and fluxes of ultraviolet emission lines at different epochs, deduced from archival IUE and GRHS/HST spectra.
Results: .The line fluxes give electron densities and were in additi…

2006 Astronomy and Astrophysics
IUE eHST 9
Faint U-Band Dropouts in the WFPC2 Parallels of the Hubble Ultra Deep Field
DOI: 10.1086/505747 Bibcode: 2006AJ....132.1023W

Casertano, Stefano; de Mello, Duilia; Wadadekar, Yogesh

We combine data from the extremely deep Hubble Space Telescope U (F300W) image, obtained using WFPC2 as part of the parallel observations of the Hubble Ultra Deep Field campaign, with BVi images from the Great Observatories Origins Deep Survey to identify a sample of Lyman break galaxies in the redshift range 2.0<~z<~3.5. We use recent stell…

2006 The Astronomical Journal
eHST 9
Evidence of standing waves during a Pi2 pulsation event observed on Cluster
DOI: 10.5194/angeo-24-2719-2006 Bibcode: 2006AnGeo..24.2719C

Blomberg, L. G.; Collier, A. B.; Hughes, A. R. W. +1 more

Observations of Pi2 pulsations at middle and low latitudes have been explained in terms of cavity mode resonances, whereas transients associated with field-aligned currents appear to be responsible for the high latitude Pi2 signature. Data from Cluster are used to study a Pi2 event observed at 18:09 UTC on 21 January 2003, when three of the satell…

2006 Annales Geophysicae
Cluster 9
Spitzer observations of red galaxies: Implication for high-redshift star formation
DOI: 10.1016/j.newar.2005.11.023 Bibcode: 2006NewAR..50..134P

Papovich, Casey

My colleagues and I identified distant red galaxies (DRGs) with J - Ks > 2.3 in the southern Great Observatories Origins Deep Surveys (GOODS-S) field. These galaxies reside at z ∼ 1-3.5, (< z> ≃ 2.2) and based on their ACS (0.4-1 µm), ISAAC (1-2.2 µm), and IRAC (3-8 µm) photometry, they typically have stellar …

2006 New Astronomy Reviews
eHST 9
Simulation of the Cluster-Spacecraft Floating Probe Potential
DOI: 10.1109/TPS.2006.883407 Bibcode: 2006ITPS...34.2078T

Escoubet, C. P.; Masson, A.; Laakso, H. +2 more

2006 IEEE Transactions on Plasma Science
Cluster 9
Saturn's Icy Moon Rhea: A Prediction for its Bulk Chemical Composition and Physical Structure at the Time of the Cassini Spacecraft First Flyby
DOI: 10.1071/AS05041 Bibcode: 2006PASA...23....1P

Prentice, Andrew J. R.

I report a model for the formation of Saturn's family of mid-sized icy moons to coincide with the first flypast of Rhea by the Cassini spacecraft on 2005 November 26. It is proposed that the moons had condensed from a concentric family of orbiting gas rings that were shed some 4.6 × 109 yr ago by the proto-Saturnian (hereafter p-Sat) cl…

2006 Publications of the Astronomical Society of Australia
Cassini 9