Search Publications

The FERRUM Project: Experimental transition probabilities of [Fe II] and astrophysical applications
DOI: 10.1051/0004-6361:20021557 Bibcode: 2003A&A...397.1143H

Lundberg, H.; Johansson, S.; Hartman, H. +9 more

We report on experimental transition probabilities for thirteen forbidden [Fe II] lines originating from three different metastable Fe Ii levels. Radiative lifetimes have been measured of two metastable states by applying a laser probing technique on a stored ion beam. Branching ratios for the radiative decay channels, i.e. M1 and E2 transitions, …

2003 Astronomy and Astrophysics
eHST 24
Tomography of a stellar X-ray corona: alpha Coronae Borealis
DOI: 10.1051/0004-6361:20030257 Bibcode: 2003A&A...403..155G

Mewe, R.; Audard, M.; Güdel, M. +1 more

We interpret the X-ray light curve obtained by XMM-Newton during a total X-ray eclipse in the nearby binary star alpha Coronae Borealis. This system consists of a G5 V main-sequence star orbiting an X-ray dark A0 star. The secondary G star is a young, active solar analog with an age of a few 100 Myr. As the primary A star eclips…

2003 Astronomy and Astrophysics
XMM-Newton 24
Stellar sources in the ISOGAL intermediate bulge fields
DOI: 10.1051/0004-6361:20030208 Bibcode: 2003A&A...403..141O

Ganesh, S.; Omont, A.; Schultheis, M. +3 more

We present a study of ISOGAL sources in the ``intermediate'' galactic bulge (|l|< 2o, |b| ~ 1o-4o), observed by ISOCAM at 7 and 15 mu m. In combination with near-infrared (I, J, Ks) data of DENIS survey, complemented by 2MASS data, we discuss the nature of the ISOGAL sources, their luminosities, the i…

2003 Astronomy and Astrophysics
ISO 24
On the measurement bias of low-l solar p-mode excitation parameters: The impact of a ground-based window function
DOI: 10.1051/0004-6361:20021627 Bibcode: 2003A&A...398..305C

Chaplin, W. J.; Elsworth, Y.; Isaak, G. R. +4 more

We present a study of the impact of a ground-based, multi-station window function on estimates of the power and damping of low-l solar p modes extracted from fits to resonant structure in the frequency domain. The window functions come from six-site observations made by the Birmingham Solar-Oscillations Network (BiSON) over the 10-yr period beginn…

2003 Astronomy and Astrophysics
SOHO 24
The association of transequatorial loops in the solar corona with coronal mass ejection onset
DOI: 10.1051/0004-6361:20021886 Bibcode: 2003A&A...400..759G

Harra, L. K.; Matthews, S. A.; Foley, C. A. +1 more

It has been shown that transequatorial loops can disappear in association with the onset of a coronal mass ejection (CME) (Khan & Hudson \cite{khan}). We extend this result by considering a larger sample of transequatorial loop systems (TLS) to investigate their associated flaring and CME activity. We find 10 of a total 18 TLS considered here …

2003 Astronomy and Astrophysics
SOHO 24
Detecting planetary transits in the presence of stellar variability. Optimal filtering and the use of colour information
DOI: 10.1051/0004-6361:20030093 Bibcode: 2003A&A...401..743C

Aigrain, S.; Favata, F.; Carpano, S.

Space-based photometric transit searches, such as the ESA mission Eddington (planned for launch in 2007), are expected to detect large numbers of terrestrial planets outside the solar system, including some Earth-like planets. Combining simplicity of concept with efficiency, the transit method consists in detecting the periodic luminosity drop in …

2003 Astronomy and Astrophysics
SOHO 24
Orbits and masses of twenty double stars discovered by Paul Couteau
DOI: 10.1051/0004-6361:20031130 Bibcode: 2003A&A...409..989D

Docobo, J. A.; Ling, J. F.

In this article we present the orbits and masses of 20 double stars discovered by P. Couteau at the Nice Observatory (France), namely WDS 01450+2703 (COU 750), 03321+4340 (1688), 03423+3141 (691), 06503+2409 (768), 12409+2708 (596),14138+3059 (606), 15390+2545 (612), 16584+3943 (1289), 17075+3810 (1291), 17221+2310 (415), 18035+ 4032 (1785), 18043…

2003 Astronomy and Astrophysics
Hipparcos 23
The INTEGRAL Mass Model - TIMM
DOI: 10.1051/0004-6361:20031403 Bibcode: 2003A&A...411L..19F

Hill, A. B.; Bird, A. J.; Dean, A. J. +8 more

The INTEGRAL Mass Model (TIMM) was started in 1995 and aimed to create a detailed geometrical model of the whole INTEGRAL satellite on computer. In parallel, a comprehensive Monte Carlo simulation code (called GGOD) has been developed. The mass model and the Monte Carlo code together enable the in-flight operation of INTEGRAL to be simulated at th…

2003 Astronomy and Astrophysics
INTEGRAL 23
Photoionized O VI absorbers toward the bright QSO HE 0515-4414
DOI: 10.1051/0004-6361:20030493 Bibcode: 2003A&A...404..449L

Reimers, D.; Baade, R.; Levshakov, S. A. +1 more

We report on detailed Monte Carlo inversion analysis of five O Vi systems from the spectrum of the bright quasar HE 0515-4414 (zem = 1.71). The associated system at zabs = 1.697 with the neutral hydrogen column density N(H I) = 4.4*E13 cm-2, shows pronounced absorption from highly ionized transitions of …

2003 Astronomy and Astrophysics
eHST 23
GRB 030227: The first multiwavelength afterglow of an INTEGRAL GRB
DOI: 10.1051/0004-6361:20031393 Bibcode: 2003A&A...411L.315C

Pian, E.; Palazzi, E.; Greiner, J. +39 more

We present multiwavelength observations of a gamma-ray burst detected by INTEGRAL (GRB 030227) between 5.3 hours and ~ 1.7 days after the event. Here we report the discovery of a dim optical afterglow (OA) that would not have been detected by many previous searches due to its faintess (R ~ 23). This OA was seen to decline follow…

2003 Astronomy and Astrophysics
INTEGRAL 23