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The massive binary CPD - 41° 7742. II. Optical light curve and X-ray observations
DOI: 10.1051/0004-6361:20052746 Bibcode: 2005A&A...441..213S

Gosset, E.; Rauw, G.; Vreux, J. -M. +4 more

In the first paper of this series, we presented a detailed high-resolution spectroscopic study of CPD - 41° 7742, deriving for the first time an orbital solution for both components of the system. In this second paper, we focus on the analysis of the optical light curve and on recent XMM-Newton X-ray observations. In the optical…

2005 Astronomy and Astrophysics
XMM-Newton 40
GRBs and the 511 keV emission of the Galactic bulge
DOI: 10.1051/0004-6361:20042215 Bibcode: 2005A&A...432..889P

Paul, J.; Cassé, M.; Parizot, E. +1 more

We consider the phenomenology of the 511 keV emission in the Galactic bulge, as recently observed by INTEGRAL, and propose a model in which the positrons are produced by gamma-ray bursts (GRB) associated with mini-starbursts in the central molecular zone (CMZ). We show that the positrons can easily diffuse across the bulge on timescales of ∼ 10

2005 Astronomy and Astrophysics
INTEGRAL 40
Links between magnetic fields and plasma flows in a coronal hole
DOI: 10.1051/0004-6361:200500029 Bibcode: 2005A&A...432L...1W

Marsch, E.; Xia, L. D.; Wiegelmann, T.

We compare the small-scale features visible in the Ne viii Doppler-shift map of an equatorial coronal hole (CH) as observed by SUMER with the small-scale structures of the magnetic field as constructed from a simultaneous photospheric magnetogram by a potential magnetic-field extrapolation. The combined data set is analysed with respect to the sma…

2005 Astronomy and Astrophysics
SOHO 40
A study of bright Southern long period variables
DOI: 10.1051/0004-6361:20041575 Bibcode: 2005A&A...431..623L

Lebzelter, T.; Hinkle, K. H.; Wood, P. R. +2 more

In this paper we present radial velocity curves of AGB variables that exhibit various kinds of anomalies: semiregular variables (SRVs) with typical mira periods, SRVs exceeding the mira 2.5 mag amplitude limit, miras with secondary maxima in their light curves, and a SRV with a long secondary period. The stars with reliable Hipparcos parallaxes fr…

2005 Astronomy and Astrophysics
Hipparcos 39
HST/WFPC2 morphologies and bar structures of field galaxies at 0.4 < z < 1
DOI: 10.1051/0004-6361:20041968 Bibcode: 2005A&A...435..507Z

Flores, H.; Hammer, F.; Assémat, F. +2 more

To address how the galaxy Hubble sequence is established and what physical processes are involved, we studied morphological properties and internal structures of field galaxies in the past (0.4<z<1). In addition to structural parameters derived from bulge+disk decomposition, Zheng et al. (2004, A&A, 421, 847) introduced color maps in rec…

2005 Astronomy and Astrophysics
eHST 39
An ISOCAM survey through gravitationally lensing galaxy clusters. IV. Luminous infrared galaxies in Cl 0024+1654 and the dynamical status of clusters
DOI: 10.1051/0004-6361:20041782 Bibcode: 2005A&A...431..433C

Kneib, J. -P.; Altieri, B.; Miville-Deschênes, M. -A. +9 more

Observations of the core of the massive cluster Cl 0024+1654, at a redshift z ∼ 0.39, were obtained with the Infrared Space Observatory using ISOCAM at 6.7 µm (hereafter 7 µm) and 14.3 µm (hereafter 15 µm). Thirty five sources were detected at 15 µm and thirteen of them are spectroscopically identif…

2005 Astronomy and Astrophysics
ISO eHST 39
On the effect of the background wind on the evolution of interplanetary shock waves
DOI: 10.1051/0004-6361:20041676 Bibcode: 2005A&A...430.1099J

Poedts, S.; Chané, E.; Jacobs, C. +1 more

The propagating shock waves in the solar corona and interplanetary (IP) space caused by fast Coronal Mass Ejections (CMEs) are simulated numerically and their structure and evolution is studied in the framework of ideal magnetohydrodynamics (MHD). Due to the presence of three characteristic velocities and the anisotropy induced by the magnetic fie…

2005 Astronomy and Astrophysics
SOHO 39
Fiber bursts as 3D coronal magnetic field probe in postflare loops
DOI: 10.1051/0004-6361:20042199 Bibcode: 2005A&A...435.1137A

Mann, G.; Aurass, H.; Rausche, G. +1 more

Fiber bursts appear in some complex solar radio bursts as a continuum fine structure in the frequency range of 150\cdots3000 MHz. We present and test a new method to use fiber bursts as a probe of the magnetic field strength and the 3D field structure in postflare loops. Thereby we assume that fiber bursts are driven by whistler waves ascending in…

2005 Astronomy and Astrophysics
SOHO 39
On the origin of microwave zebra pattern
DOI: 10.1051/0004-6361:20048337 Bibcode: 2005A&A...431.1037A

Kuznetsov, A. A.; Yan, Yihua; Altyntsev, A. T. +2 more

The results of the first observations of a zebra pattern at frequencies around5.6GHz are presented. The fine structures in the emission spectrum were recorded simultaneously by the Siberian Solar Radiotelescope and the spectropolarimeters of the National Astronomical Observatories, which allowed us to study the presented event with high spatial, t…

2005 Astronomy and Astrophysics
SOHO 39
Highly ionized gas in the local ISM: Some like it hot?
DOI: 10.1051/0004-6361:20042611 Bibcode: 2005A&A...436..615W

Lallement, R.; Welsh, B. Y.

We present HST-STIS medium-resolution spectra (R ∼ 6.5 km s-1) of the ultraviolet interstellar absorption lines observed towards 4 early-type stars located within the local interstellar medium (ISM), with sight-line distances <186 pc in the general direction of the Loop I superbubble (l = 330°, b = +18°). These data have been supplem…

2005 Astronomy and Astrophysics
eHST 38