Issue |
A&A
Volume 405, Number 1, July I 2003
|
|
---|---|---|
Page(s) | 285 - 290 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20030674 | |
Published online | 16 June 2003 |
Long-term X-ray variability of the microquasar system LS 5039/RX J1826.2-1450
1
G.A.C.E., Institut de Ciències dels Materials, Universitat de Valencia, 46071 Paterna-Valencia, Spain e-mail: pablo.reig@uv.es
2
Departament d'Astronomia i Meteorologia, Universitat de Barcelona, Av. Diagonal 647, 08028 Barcelona, Spain e-mail: mribo@am.ub.es; josep@am.ub.es
3
Departamento de Física, Escuela Politécnica Superior, Universidad de Jaén, Virgen de la Cabeza 2, 23071 Jaén, Spain e-mail: jmarti@ujaen.es
Corresponding author: P. Reig, pablo.reig@uv.es
Received:
14
February
2003
Accepted:
16
April
2003
We report on the results of the spectral and timing analysis of a BeppoSAX
observation of the microquasar system LS 5039/RX J1826.2-1450. The source was found in a low-flux state with FX(1–10 keV) = erg cm-2 s-1, which represents almost one order of magnitude
lower than a previous RXTE observation 2.5 years before. The 0.1–10 keV
spectrum is described by an absorbed power-law continuum with
photon-number spectral index
and hydrogen column
density of
cm-2.
According to the orbital parameters of the system, the BeppoSAX
observation covers the time of an X-ray eclipse should one occur.
However, the 1.6–10 keV light curve does not show evidence of such an
event, which allows us to give an upper limit to the inclination of the
system. The low X-ray flux detected during this observation is interpreted
as a decrease in the mass accretion rate onto the compact object due to a
decrease in the mass-loss rate from the primary.
Key words: stars: individual: LS 5039, RX J1826.2-1450, 3EG J1824-1514 / X-rays: stars / stars: variables: general / radio continuum: stars
© ESO, 2003
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