Search Publications

Models for the positive latitude e{-}e{+} annihilation feature
DOI: 10.1051/0004-6361:20021527 Bibcode: 2003A&A...397..635V

Knödlseder, J.; Guessoum, N.; Jean, P. +1 more

Galactic maps of e-e+ annihilation radiation based on CGRO-OSSE, SMM and TGRS data have indicated the existence of an extended component at positive Galactic latitudes (l~ -2 deg, b~ 7 deg), in addition to the emission from the galactic bulge and disk (Purcell et al. \cite{Purcell97}; Cheng et al. \cite{…

2003 Astronomy and Astrophysics
INTEGRAL 13
The Long Aftermath of Superoutbursts: STIS Results on AL Comae 5.5 Years Past Outburst
DOI: 10.1086/377022 Bibcode: 2003AJ....126.1451S

Szkody, Paula; Howell, Steve B.; Sion, Edward M. +2 more

The Space Telescope Imaging Spectrograph (STIS) was used to obtain the ultraviolet spectrum of AL Comae 5.5 yr past its 1995 April superoutburst. The spectrum can be fitted by a model of a logg=8+/-0.5 white dwarf with a temperature of 16,300+/-1000 K. Surprisingly, the flux distribution is exactly the same as the Faint Object Spectrograph data ob…

2003 The Astronomical Journal
eHST 13
GRB 021219: The first Gamma-Ray Burst localized in real time with IBAS
DOI: 10.1051/0004-6361:20031303 Bibcode: 2003A&A...411L.311M

Götz, D.; Mereghetti, S.; von Kienlin, A. +5 more

On December 19, 2002, during the Performance and Verification Phase of INTEGRAL, a Gamma-Ray Burst (GRB) has been detected and localized in real time with the INTEGRAL Burst Alert System (IBAS). Here we present the results obtained with the IBIS and SPI instruments. The burst had a time profile with a single peak lasting about 6 s. The peak spectr…

2003 Astronomy and Astrophysics
INTEGRAL 13
The Input Catalogue for the OMC camera onboard INTEGRAL
DOI: 10.1051/0004-6361:20031400 Bibcode: 2003A&A...411L.281D

Mas-Hesse, J. M.; Jordi, C.; Figueras, F. +6 more

The Optical Monitoring Camera (OMC) onboard INTEGRAL (launched on October 17, 2002) has been designed to obtain V-Johnson photometry simultaneously with high energy observations at X-ray (3-35 keV) and gamma-ray (15 keV-10 MeV) performed by the main instruments onboard INTEGRAL. Due to technical limitations on the data processing electronics and t…

2003 Astronomy and Astrophysics
INTEGRAL 13
Coronal mass ejection interaction and particle acceleration during the 2001 April 14 15 events
DOI: 10.1016/j.asr.2003.09.038 Bibcode: 2003AdSpR..32.2613G

Kaiser, M. L.; Howard, R. A.; Gopalswamy, N. +1 more

Two successive solar energetic particle (SEP) events associated with fast and wide coronal mass ejections (CMEs) on 2001 April 14 and 15 are compared. The weak SEP event of April 14 associated with an 830 km/s CME and an M1.0 flare was the largest impulsive event of cycle 23. The April 15 event, the largest ground level event of cycle 23, was thre…

2003 Advances in Space Research
SOHO 13
A high-resolution radio study of neutral gas in the starburst galaxy NGC 520
DOI: 10.1046/j.1365-2966.2003.07104.x Bibcode: 2003MNRAS.346..424B

Beswick, R. J.; Pedlar, A.; Clemens, M. S. +1 more

We present subarcsec angular resolution observations of the neutral gas in the nearby starburst galaxy NGC 520. The central kpc region of NGC 520 contains an area of significantly enhanced star formation. The radio continuum structure of this region resolves into ~10 continuum components. By comparing the flux densities of the brightest of these c…

2003 Monthly Notices of the Royal Astronomical Society
eHST 13
2D MHD modelling of compressible and heated coronal loops obtained via nonlinear separation of variables and compared to TRACE and SoHO observations
DOI: 10.1051/0004-6361:20031001 Bibcode: 2003A&A...409.1065P

Gontikakis, C.; Tsinganos, K.; Aschwanden, M. J. +2 more

An analytical MHD model of coronal loops with compressible flows and including heating is compared to observational data. The model is constructed via a systematic nonlinear separation of the variables method used to calculate several classes of exact MHD equilibria in Cartesian geometry and uniform gravity. By choosing a particularly versatile so…

2003 Astronomy and Astrophysics
SOHO 13
Variability of The Old Nova V603 Aquilae in UV and X-ray bands
DOI: 10.1051/0004-6361:20030390 Bibcode: 2003A&A...405..663B

Szkody, P.; Schwarzenberg-Czerny, A.; Borczyk, W.

We present the results of a campaign of simultaneous observations of V603 Aql in the X-ray and UV bands accomplished with the IUE and ROSAT satellites. Simultaneous observations cover 20 orbital cycles, while the total span of all the observations is 40 cycles. This constitutes the longest continuous UV time series of simultaneous space observatio…

2003 Astronomy and Astrophysics
IUE 13
Atomic Data and Spectral Line Intensities for S X
DOI: 10.1086/375721 Bibcode: 2003ApJS..147..409B

Bhatia, A. K.; Landi, E.

Electron impact collision strengths, energy levels, oscillator strengths and spontaneous radiative decay rates are calculated for S X. The configurations included are 2s22p3, 2s2p4, 2p5, 2s22p23s, 2s22p23p, and 2s22p23d giving rise to 72 f…

2003 The Astrophysical Journal Supplement Series
SOHO 13
The microwave subsecond pulse of September 17, 2001: The spectrum, location and size of the source
DOI: 10.1051/0004-6361:20021905 Bibcode: 2003A&A...400..337A

Yan, Yihua; Altyntsev, A. T.; Meshalkina, N. S. +2 more

We examine simultaneous observations of microwave subsecond pulses with high temporal, spatial and spectral resolution from the Siberian Solar Radio Telescope (5.7 GHz, 14 ms resolution) and from the spectropolarimeters (5.2-7.6 GHz, 6 ms) of the National Astronomical Observatories. The September 17, 2001 flare is discussed in detail. The subsecon…

2003 Astronomy and Astrophysics
SOHO 13