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XMM-Newton observations of the supernova remnant RX J1713.7-3946 and its central source
DOI: 10.1051/0004-6361:20041154 Bibcode: 2004A&A...427..199C

Ballet, J.; Decourchelle, A.; Giacani, E. +3 more

We present new results from the observations of the supernova remnant (SNR) RX J1713.7-3946 (also G347.3-0.5) performed in five distinct pointings with the EPIC instrument on board the satellite XMM-Newton. RX J1713.7-3946 is a shell-type SNR dominated by synchrotron radiation in the X-rays. Its emission (emis…

2004 Astronomy and Astrophysics
XMM-Newton 133
A Numerical Model of a Coronal Mass Ejection: Shock Development with Implications for the Acceleration of GeV Protons
DOI: 10.1086/392504 Bibcode: 2004ApJ...605L..73R

Gombosi, T. I.; Roussev, I. I.; Lee, M. A. +3 more

The initiation and evolution of the coronal mass ejection, which occurred on 1998 May 2 in NOAA Active Region 8210, are modeled using a fully three-dimensional, global MHD code. The initial magnetic field for the model is based on magnetogram data from the Wilcox Solar Observatory, and the solar eruption is initiated by slowly evolving the boundar…

2004 The Astrophysical Journal
SOHO 133
GEMS Imaging of Red-Sequence Galaxies at z~0.7: Dusty or Old?
DOI: 10.1086/381388 Bibcode: 2004ApJ...600L..11B

Bell, Eric F.; Somerville, Rachel S.; Wisotzki, Lutz +13 more

We have used the 30'×30' Hubble Space Telescope image mosaic from the Galaxy Evolution from Morphology and Spectral energy distributions (GEMS) project in conjunction with the COMBO-17 deep photometric redshift survey to define a sample of nearly 1500 galaxies with 0.65<=z<=0.75. With this sample, we can study the distr…

2004 The Astrophysical Journal
eHST 133
Dynamics of solar coronal loops. II. Catastrophic cooling and high-speed downflows
DOI: 10.1051/0004-6361:20040403 Bibcode: 2004A&A...424..289M

Peter, H.; Hansteen, V. H.; Müller, D. A. N.

This work addresses the problem of plasma condensation and ``catastrophic cooling'' in solar coronal loops. We have carried out numerical calculations of coronal loops and find several classes of time-dependent solutions (static, periodic, irregular), depending on the spatial distribution of a temporally constant energy deposition in the loop. Dyn…

2004 Astronomy and Astrophysics
SOHO 131
Long-Term Cosmic-Ray Modulation in the Heliosphere
DOI: 10.1086/381649 Bibcode: 2004ApJ...603..744F

Ferreira, S. E. S.; Potgieter, M. S.

A time-dependent model based on a numerical solution of Parker's transport equation is used to model the modulation of cosmic-ray protons, electrons, and helium for full 11 year and 22 year modulation cycles using a compound approach. This approach incorporates the concept of propagating diffusion barriers, increases in the heliospheric magnetic f…

2004 The Astrophysical Journal
Ulysses 131
The nature of the Galactic Center source IRS 13 revealed by high spatial resolution in the infrared
DOI: 10.1051/0004-6361:20034147 Bibcode: 2004A&A...423..155M

Rigaut, F.; Paumard, T.; Stolovy, S. R. +1 more

High spatial resolution observations in the 1 to 3.5 µm/ region of the Galactic Center source known historically as IRS 13 are presented. They include ground-based adaptive optics images in the H, Kp (2.12/0.4 µm) and L bands, HST-NICMOS data in filters between 1.1 and 2.2 µm, and integral field spectroscopic d…

2004 Astronomy and Astrophysics
eHST 131
A review of the distance and structure of the Large Magellanic Cloud
DOI: 10.1016/j.newar.2004.03.001 Bibcode: 2004NewAR..48..659A

Alves, David R.

The average of 14 recent measurements of the distance to the Large Magellanic Cloud (LMC) implies a true modulus of 18.50 ± 0.02 mag, and demonstrates a trend in the past 2 years of convergence toward a standard value. The distance indicators reviewed are the red clump, the tip of the red giant branch, Cepheid, RR Lyrae, and Mira variable stars, c…

2004 New Astronomy Reviews
eHST 130
The XMM-Newton Iron Line Profile of NGC 3783
DOI: 10.1086/381091 Bibcode: 2004ApJ...602..648R

Nandra, K.; Turner, T. J.; Reeves, J. N. +3 more

We report on observations of the iron K line in the nearby Seyfert 1 galaxy, NGC 3783, obtained in a long, two-orbit (~240 ks) XMM-Newton observation. The line profile obtained exhibits two strong narrow peaks at 6.4 and 7.0 keV, with measured line equivalent widths of 120 and 35 eV, respectively. The 6.4 keV emission is the Kα line from near neut…

2004 The Astrophysical Journal
XMM-Newton 130
A Constant Bar Fraction out to Redshift z ~ 1 in the Advanced Camera for Surveys Field of the Tadpole Galaxy
DOI: 10.1086/422407 Bibcode: 2004ApJ...612..191E

Elmegreen, Bruce G.; Elmegreen, Debra Meloy; Hirst, Amelia C.

Barlike structures were investigated in a sample of 186 disk galaxies larger than 0.5" that are in the I-band image of the Tadpole galaxy taken with the Hubble Space Telescope Advanced Camera for Surveys. We found 22 clear cases of barred galaxies, 21 galaxies with small bars that appear primarily as isophotal twists in a contour plot, and 11 case…

2004 The Astrophysical Journal
eHST 129
Cluster observations of earthward flowing plasmoid in the tail
DOI: 10.1029/2004GL020692 Bibcode: 2004GeoRL..3118803Z

Balogh, A.; Glassmeier, K. -H.; Zhang, H. +10 more

The energetic electrons and ions embedded in Earthward-moving plasmoid structures have been observed. These plasmoids are associated with a rotational local Bz component (bi-polar) signature. Energetic electrons are found to be confined in a smaller spatial region than ions inside the plasmoid. Energetic ions and electrons seem to be a …

2004 Geophysical Research Letters
Cluster 129