Search Publications

Abell 851: Are we looking at the beginning of a merging process?
DOI: 10.1023/A:1024690632590 Bibcode: 2003Ap&SS.285..167D

Schindler, S.; De Filippis, E.

We present an XMM observation of the moderately distant (z=0.41)galaxy cluster CL 0939+4713 (Abell 851), an exceptionally rich cluster. The formation and evolution of clusters depends sensitively on cosmological parameters like the mean matter density in the universe Οm. Therefore it is important to determine the dynamical state of clus…

2003 Astrophysics and Space Science
XMM-Newton 1
On the importance of searching for oscillations of the Jovian inner radiation belt with a quasi-period of 40 minutes
DOI: 10.1046/j.1365-8711.2003.06987.x Bibcode: 2003MNRAS.344L...1L

Lou, Yu-Qing; Zheng, Chen

Experiments aboard the Ulysses spacecraft discovered quasi-periodic bursts of relativistic electrons and of radio emissions with ~40-min period (QP-40) from the south polar direction of Jupiter in 1992 February. Such polar QP-40 burst activities were found to correlate well with arrivals of high-speed solar winds at Jupiter. We advance the physica…

2003 Monthly Notices of the Royal Astronomical Society
Ulysses 1
Testing SPI imaging of high-energy and extended sources
DOI: 10.1051/0004-6361:20031394 Bibcode: 2003A&A...411L.101W

Strong, A. W.; Wunderer, C. B.; Connell, P. +2 more

INTEGRAL's main instruments employ coded apertures to obtain directional information on the incoming radiation. In order to experimentally better determine the imaging capabilities of the spectrometer SPI, the SPI Imaging Test Setup (SPITS) has been built at MPE. It consists of the SPI coded mask and two SPI-identical Ge detectors on an XY-table w…

2003 Astronomy and Astrophysics
INTEGRAL 1
XMM-Newton high-resolution x-ray spectroscopy of the Wolf-Rayet object WR25 (WN6HA+04F)
DOI: 10.1016/S0273-1177(03)00323-5 Bibcode: 2003AdSpR..32.1161R

Schmutz, W.; Raassen, A. J. J.; Mewe, R. +5 more

We report the analysis of the X-ray spectrum of the Wolf-Rayet star WR 25, observed by RGS and EPIC-MOS on board XMM-Newton. Temperatures up to 40 MK have been determined. Strong absorption, exceeding the value due to the Inter Stellar Medium (ISM) has been detected and assigned to the dense stellar wind.

2003 Advances in Space Research
XMM-Newton 1
The system of the Milky Way, LMC and SMC
DOI: 10.1023/A:1024068613813 Bibcode: 2003Ap&SS.284..519R

Ružčka, Adam

A simple sticky-particle numerical model has been developed in order to check whether extended structures of gas created due to the dynamical evolution of the Galaxy and the Magellanic Clouds system can be explained as remnants of a tidal interaction. Influence of dissipative nature of gaseous medium has been taken into account. The most remarkabl…

2003 Astrophysics and Space Science
Hipparcos 1
X-ray emission from dwarf galaxies: IC 2574 revisited
DOI: 10.1023/A:1024026610546 Bibcode: 2003Ap&SS.284..627B

Walter, Fabian; Brinks, Elias; Kerp, Jürgen

Until recently, few unequivocal detections had been reported of the hot, X-ray emitting gas thought to be associated with the large, coherent structures variously described as supershells or superbubbles in dwarf irregular (dIrr) galaxies. In this contribution we report follow-up XMM-Newton and Chandra observations of our ROSAT detection of X-ray …

2003 Astrophysics and Space Science
XMM-Newton 1
The Mass/Eccentricity Limit in Double Star Astronomy
DOI: 10.1007/BF02702315 Bibcode: 2003JApA...24...99D

Dommanget, J.

A research that we conducted in 1963 on the evolution of the binaries based on the available orbital data to obtain a philosophical degree, led to the establishment of an interesting and new diagram between the logarithm of the total mass and a particular parameterX, bound to the areal constant. This appeared to have a real physical significance b…

2003 Journal of Astrophysics and Astronomy
Hipparcos 1
The complex structure of the Mg II regions of 40 BeV stars
Bibcode: 2003POBeo..76...27L

Danezis, E.; Lyratzi, E.; Theodossiou, E. +4 more

In this paper we present a study of the UV Mg II resonance lines in 40 BeV stars' spectra. We used the model proposed by Danezis et al. (2002, 2003). This model is based on the idea of independent density layers in the regions where the spectral lines that present SACs (DACs) are created. We calculated the apparent rotation (Vrot) and e…

2003 Publications de l'Observatoire Astronomique de Beograd
IUE 1
INTEGRAL surveys
DOI: 10.1002/asna.200310059 Bibcode: 2003AN....324..160W

Walter, R.; Kretschmar, P.; Paizis, A. +2 more

2003 Astronomische Nachrichten
INTEGRAL 1
The XMM large-scale structure survey: scientific motivation and first cluster candidates
DOI: 10.1002/asna.200310032 Bibcode: 2003AN....324..124V

Valtchanov, I.; Pierre, M.

The XMM-Newton Large-Scale Structure Survey (XMM-LSS) will ultimately cover a region of 8x8 square degrees and with the unprecedented sensitivity of XMM will provide a unique dataset to study the evolution of the cosmic network as traced by clusters and AGNs/QSOs. We discuss the scientific goals and show some first observations of candidate cluste…

2003 Astronomische Nachrichten
XMM-Newton 1