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AD Leonis, (dM3:l5V): Analysis of the x-ray spectrum
DOI: 10.1016/S0273-1177(03)00322-3 Bibcode: 2003AdSpR..32.1155V

Raassen, A. J. J.; Mewe, R.; Audard, M. +3 more

We report the analysis of the X-ray spectrum of AD Leo (dM3.5 V), observed by RGS and EPIC-MOS on board XMM-Newton and by LETGS on board Chandra. From the lightcurve the presence of flaring states and a quiescent part is noticed. Temperatures up to 20 MIA have been determined. A significant increase of the emission measure (EM) at high temperature…

2003 Advances in Space Research
XMM-Newton 0
Broad Iron Lines in Active Galactic Nuclei
DOI: 10.1088/1009-9271/3/S1/157 Bibcode: 2003ChJAS...3..157W

Reynolds, C. S.; Kendziorra, E.; Wilmsn, J.

The Fe Kα lines seen in many Active Galactic Nuclei (AGN) are thought to originate close to the central supermassive black hole. In this review we summarize the physics of the fluorescent line formation and show that Fe Kα line profile observations can be used to probe relativistic effects in the vicinity of the black hole, concentrating on recent…

2003 Chinese Journal of Astronomy and Astrophysics Supplement
XMM-Newton 0
Erratum: XMM-Newton view of the Hubble Deep Field-North and Groth-Westphal Strip regions
DOI: 10.1002/asna.200310199 Bibcode: 2003AN....324..506M

Griffiths, R. E.; Miyaji, T.; Lumb, D. +2 more

In the paper, ``XMM-Newton view of the Hubble Deep Field-North and Groth-Westphal strip regions'' by Miyaji et al. (2003), we found that one of the data points on Fig. ref{fig:lnls} was incorrectly plotted. The corrected figure is shown below.

2003 Astronomische Nachrichten
XMM-Newton 0
Multifrequency study of the very slow nova V723 Cas
DOI: 10.1088/1009-9271/3/S1/341 Bibcode: 2003ChJAS...3..341C

Chochol, D.; Vittone, A. A.; Pribulla, T.

Multifrequency behaviour of the very slow nova V723 Cas is reviewed. The long-term photometry of the object revealed the orbital period 0.693265 days of the binary, quasi-periodic oscillations in the envelope of the burst white dwarf and 182 days periodicity of activity due to the mass transfer bursts from the red to the white dwarf probably cause…

2003 Chinese Journal of Astronomy and Astrophysics Supplement
IUE 0
A survey of 3He enhancements at 2-20 MeV/nucleon: Ulysses COSPIN/LET observations
DOI: 10.5194/angeo-21-1245-2003 Bibcode: 2003AnGeo..21.1245T

Sanderson, T. R.; Marsden, R. G.; Tranquille, C. +1 more

We present the results of a survey of enhancements in the ratio of 3He/4 He as measured by the COSPIN/LET instrument on board the Ulysses spacecraft in the energy range 2-20 MeV/n. In the context of this study, all ratios of 3He/4 He above 0.05 are considered to be enhanced compared with the solar system value of ~0.0004. Previous studies have sho…

2003 Annales Geophysicae
Ulysses 0
Role of low-frequency modes in organizing the inner heliosphere
DOI: 10.1029/2001JA000058 Bibcode: 2003JGRA..108.1107H

Kunow, H.; Heber, B.; Lanzerotti, Louis J. +2 more

Cosmic ray proton data (125 to >2000 MeV) measured in the inner three-dimensional (3-D) heliosphere over the years from 1993 into 2000 by the KET instrument on the Ulysses spacecraft are examined. The data are parameterized and characterized by fitting products of spherical harmonic and sinusoidal frequency functions to three individual proton …

2003 Journal of Geophysical Research (Space Physics)
Ulysses 0
Optical and UV Spectral Diagnostics for GPS and CSS Sources
DOI: 10.1071/AS02026 Bibcode: 2003PASA...20...31D

Dopita, Michael A.

In this paper I examine the use of optical and UV spectral diagnostic ratios to distinguish between gas which is locally shock-excited by the interaction with a jet and that which is photoionised by the central engine. In many cases key UV lines remain unobserved except in the case of high redshift radio galaxies. However, in one case, the nearby …

2003 Publications of the Astronomical Society of Australia
eHST 0
Fuzzy set theory applied to CME importance classification
DOI: 10.1016/S0275-1062(03)90052-X Bibcode: 2003ChA&A..27..303H

Han, Zheng-Zhong; Tang, Yu-Hua

In this paper, fuzzy set theory is applied to a quantitative way of assigning importance class to coronal mass ejection (CME) events based on four observed characteristics, i.e. velocity, span, mass and kinetic energy. The weights to be associated with each of the characteristics and the membership functions of belonging to one of the three import…

2003 Chinese Astronomy and Astrophysics
SOHO 0
Cosmic Ray Drifts at Solar Maximum
Bibcode: 2003ICRC....7.3807F

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

A fully time-dep endent cosmic ray modulation model, based on the numerical solution of Parker's transport equation, is used to study the amount of particle drifts needed to explain the observed 2.5 GV electron to proton ratio (e/p) by the KET instrument on the Ulysses spacecraft. It is shown that the model successfully simulates the modulation of…

2003 International Cosmic Ray Conference
Ulysses 0
Reduction of ringing effects by an improved deconvolution algorithm. Application to A370 CFHT image of gravitational arcs
DOI: 10.1051/0004-6361:20031111 Bibcode: 2003A&A...409..387R

Mellier, Y.; Aime, C.; Roche, M. +2 more

We develop a self-consistent automatic procedure to restore information from astronomical observations. It relies on both a new deconvolution algorithm called LBCA (Lower Bound Constraint Algorithm) and the use of the Wiener filter. In order to explore its scientific potential for strong and weak gravitational lensing, we process a CFHT image of t…

2003 Astronomy and Astrophysics
eHST 0