Search Publications

Gamma-ray observations of explosive nucleosynthesis products
DOI: 10.1016/j.asr.2005.01.097 Bibcode: 2005AdSpR..35..976V

Vink, Jacco

In this review I discuss the various γ-ray emission lines that can be expected and, in some cases have been observed, from radioactive explosive nucleosynthesis products. The most important γ-ray lines result from the decay chains of 56Ni, 57Ni, and 44Ti. 56Ni is the prime explosive nucleosynthesis produ…

2005 Advances in Space Research
INTEGRAL 26
A mapping of martian water sublimation during early northern summer using OMEGA/Mars Express
DOI: 10.1051/0004-6361:200500171 Bibcode: 2005A&A...441L...9E

Bibring, J. -P.; Gondet, B.; Langevin, Y. +8 more

The OMEGA imaging spectrometer aboard Mars Express has been used to map the water vapor abundance over the martian surface, from the analysis of the 2.6 µm band of H2O. As a preliminary result of this study, we present water vapor maps in the northern hemisphere at the time of the northern polar cap sublimation (Ls = 94-112 deg). The maps sh…

2005 Astronomy and Astrophysics
MEx 26
Discovery of X-ray eclipses from the transient source CXOGC J174540.0-290031 with XMM-Newton
DOI: 10.1051/0004-6361:20053214 Bibcode: 2005A&A...443..571P

Grosso, N.; Warwick, R. S.; Porquet, D. +4 more

We present the XMM-Newton observations obtained during four revolutions in Spring and Summer 2004, of CXOGC J174540.0-290031, a moderately bright transient X-ray source, located at only 2.9'' from Sgr A*. We report the discovery of sharp and deep X-ray eclipses, with a period of 27 961±5 s and a duration of about 1100±100 s, observed during the tw…

2005 Astronomy and Astrophysics
XMM-Newton 26
The heliospheric modulation of 3 10 MeV electrons: Modeling of changes in the solar wind speed in relation to perpendicular polar diffusion
DOI: 10.1016/j.asr.2005.03.123 Bibcode: 2005AdSpR..35..597M

Fichtner, H.; Ferreira, S. E. S.; Potgieter, M. S. +3 more

The discrepancy between cosmic ray model predictions representing solar minimum conditions in the heliosphere and the 3-10 MeV post-1998 electrons observations by the Kiel Electron Telescope (KET) onboard Ulysses suggests the need for consistent changes in model parameters with increasing solar activity. In order to reduce this discrepancy, an eff…

2005 Advances in Space Research
Ulysses 26
Observations of Hα Intensity Oscillations in a Flare Ribbon
DOI: 10.1086/427084 Bibcode: 2005ApJ...620.1101M

Gallagher, Peter T.; Mathioudakis, Mihalis; Bloomfield, D. Shaun +6 more

High-cadence Hα blue wing observations of a C9.6 solar flare obtained at Big Bear Solar Observatory using the Rapid Dual Imager are presented. Wavelet and time-distance methods were used to study oscillatory power along the ribbon, finding periods of 40-80 s during the impulsive phase of the flare. A parametric study found statistically significan…

2005 The Astrophysical Journal
SOHO 26
Transient Coronal Holes as Seen in the He I 1083 nm MLSO Observations
DOI: 10.1086/426904 Bibcode: 2005ApJ...621.1109D

de Toma, G.; Holzer, T. E.; Burkepile, J. T. +1 more

Observations from Yohkoh SXT and SOHO EIT have shown that dimming regions often appear on the solar disk near the location of a coronal mass ejection (CME). We now can see brightenings in He I 1083 nm observations made at the Mauna Loa Solar Observatory (MLSO) that form at the same time and are cospatial with the EUV intensity dimmings observed fr…

2005 The Astrophysical Journal
SOHO 26
Recovery of the Orbital Parameters and Pulse Evolution of V0332+53 during a Huge Outburst
DOI: 10.1086/462415 Bibcode: 2005ApJ...630L..65Z

Torres, Diego F.; Zhang, Shu; Qu, Jin-Lu +1 more

The high-mass X-ray binary V0332+53 became active at the end of 2004, and the outburst was observed in hard X-rays by RXTE and INTEGRAL. Based on these hard X-ray observations, we measure the orbital parameters by fitting the Doppler-shifted spin periods. The derived orbital period and eccentricity are consistent with those obtained by Stella et a…

2005 The Astrophysical Journal
Exosat INTEGRAL 26
Physical Conditions in the Narrow-Line Region of Markarian 3. I. Observational Results
DOI: 10.1086/426314 Bibcode: 2005ApJ...619..116C

Collins, Nicholas R.; Crenshaw, D. Michael; Bruhweiler, Frederick C. +3 more

We use Hubble Space Telescope Space Telescope Imaging Spectrograph (STIS) long-slit low-resolution spectroscopy from 1150 to 10300 Å to study the physical conditions in the narrow-line region (NLR) of the Seyfert 2 galaxy Markarian 3. We find from the He II λ1640/λ4686 line ratio and the Balmer decrement that the extinction within Mrk 3 along the …

2005 The Astrophysical Journal
eHST 26
Discovery of Photospheric Germanium in Hot DA White Dwarfs
DOI: 10.1086/429667 Bibcode: 2005ApJ...622L.121V

Vennes, Stéphane; Chayer, Pierre; Dupuis, Jean

We report the identification of Ge IV resonance lines in ultraviolet spectra of the hot DA white dwarfs Feige 24, G191-B2B, and GD 246. The lines originate in the stellar photosphere, and we measure low Ge/H abundance ratios ranging between -8.0 and -8.7. We also tentatively identify a resonance line of Sn IV blended with an Fe V line in the spect…

2005 The Astrophysical Journal
IUE eHST 26
Morphology and geological structure of the western part of the Olympus Mons volcano on Mars from the analysis of the Mars Express HRSC imagery
DOI: 10.1007/s11208-005-0025-2 Bibcode: 2005SoSyR..39...85B

Jaumann, R.; Head, J. W.; Neukum, G. +8 more

The images of the western part of Olympus Mons and adjacent plains acquired by the HRSC camera onboard the Mars Express spacecraft were studied. The morphology, topography, and color of the surface were investigated. The surface age was determined by the frequencies of impact craters. The examination of the HRSC images combined with an analysis of…

2005 Solar System Research
MEx 26