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Physical parameters of helium-rich subdwarf B stars from spectral energy distributions
Jeffery, C. S.; Ahmad, A.
We present effective temperatures and angular radii for eleven helium-rich subdwarf B stars. These are measured using spectral energy distributions from archival IUE spectra and existing optical and infrared photometry. The data have been analysed using a grid of high-gravity helium-rich LTE model atmospheres and a χ2-minimization proce…
XMM-Newton surveys of the Canada-France Redshift Survey fields - II. The X-ray catalogues, the properties of the host galaxies and the redshift distribution
Nandra, K.; Lilly, S.; McCracken, H. J. +5 more
We present the X-ray source catalogues for the XMM surveys of the 3-h and 14-h Canada-France Redshift Survey fields (0.5-10 keV flux range ~2 × 10-15-10-13 erg cm-2 s-1). We use a subset of the XMM sources, which have Chandra positions, to determine the best method of obtaining optical identifications of…
Statistical behavior of foreshock Langmuir waves observed by the Cluster wideband data plasma wave receiver
Balogh, A.; Lucek, E.; Gurnett, D. +3 more
Available from http://www.copernicus.org/site/EGU/annales/22/7/2337.htm?FrameEngine=false;
Mafic silicate mapping on Mars: effects of palagonitic material, multiple mafic silicates, and spectral resolution
Bell, James F.; Cloutis, Edward A.
The visible to near-infrared spectral reflectance properties of intimate and areal pyroxene + palagonitic material mixtures as well as pure mafic silicates (low-calcium pyroxene, high-calcium pyroxene, pigeonite, olivine) and mixtures of these minerals were analyzed at high spectral resolution (5 nm) as well as with non-contiguous band passes equi…
High-resolution far ultraviolet spectrum of electron-excited SO2
Ajello, Joseph; Bhardwaj, Anil; Vatti Palle, Prahlad
The high-resolution UV capabilities (λ/Δλ = 105) of the Hubble Space Telescope (HST) equipped with the Space Telescope Imaging Spectrograph (STIS) reflects a need for a high-resolution laboratory UV spectral data base for comparison with observation. For the purpose of interpreting the astronomical observations of Io by HST the electron…
Estimating stellar parameters from spectra. I. Goodness-of-fit parameters and lack-of-fit test
Aerts, C.; Decin, L.; Molenberghs, G. +2 more
Estimating stellar parameters from spectrophotometric data is a key tool in the study of stellar structure and stellar evolution. Although many methods have been proposed to estimate stellar parameters from ultraviolet (UV), optical and infrared (IR) data using low, medium or high-resolution observational data of the target(s), only a few address …
XMM-Newton observations of the Vela pulsar
Zane, S.; Hailey, C. J.; Mori, K. +1 more
We present spectral analysis from XMM-Newton observations of the Vela pulsar. We analyzed thermal emission from the pulsar dominating below ~1 keV since extracted spectra are heavily contaminated by nebular emission at higher energy. Featureless high-resolution spectra of the reflection grating spectrometer aboard XMM-Newton suggest the presence o…
Preliminary Orbits for Eight Visual Binaries
Ling, J. F.
This paper reports orbits and masses calculated for the visual binary stars WDS 00427-6537 (I440), WDS 01084-5515 (RST 1205 AB), WDS 01343-0827 (A314), WDS 03590+0947 (HU 27), WDS 10287+4558 (A1993), WDS 12429+0516 (A1602), WDS 20157+4339 (A2095 AB), and WDS 22180-6249 (I20). All the orbits have previously been announced in IAU Commission 26 Infor…
Proper motions of open star clusters from Tycho-2 catalogue data
Beshenov, G. V.; Loktin, A. V.
The results of determinating the proper motions of open clusters on the basis of the Tycho-2 catalogue data are presented here. The resulting catalogue contains mean proper motions for 390 open clusters.
Investigation of the source region of ionospheric oxygen outflow in the cleft/cusp using multi-spacecraft observations by CIS onboard Cluster
Lundin, R.; Dandouras, I.; Klecker, B. +18 more
Beams of singly ionized oxygen with narrow energy distributions originating in the dayside cleft/cusp region are frequently observed in the cleft, cusp and polar cap regions by the CODIF sensor of the CIS instrument onboard Cluster. During summer and fall of 2001, the high separation distances of ∼1 Re between the spacecraft provided a good opport…