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Confirmation of persistent radio jets in the microquasar LS 5039,
J.M. Paredes, M. Ribó, E. Ros, M. Massi, & J. Martí
Astronomy & Astrophysics, submitted (2002)
- Abstract
We present here new observations conducted with the EVN and MERLIN of the
persistent microquasar LS 5039 discovered by Paredes et al.
(2000) with the VLBA. The new observations confirm the presence of
an asymmetric two-sided jet reaching
up to ~1000 AU on the longest jet
arm. The results suggest a bending of the jets with increasing distance from
the core and/or precession. The origin and location of the high-energy
gamma-ray emission associated with the system is discussed and an estimate of
the magnetic field at the basis of the jet given. Our results suggest a well
collimated radio jet. We also comment on new observing strategies to be used
with satellites and forthcoming detectors, since this source
appears to be a rather good laboratory to explore the accretion/ejection
processes taking place in microquasars.
Eduardo Ros
ros@mpifr-bonn.mpg.de