Open AccessFirst e‐VLBI observations of Cygnus X‐3
Author(s) -
Tudose V.,
Fender R. P.,
Garrett M. A.,
MillerJones J. C. A.,
Paragi Z.,
Spencer R. E.,
Pooley G. G.,
Van Der Klis M.,
Szomoru A.
Publication year - 2007
Publication title -
monthly notices of the royal astronomical society: letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.067
H-Index - 122
eISSN - 1745-3933
pISSN - 1745-3925
DOI - 10.1111/j.1745-3933.2006.00264.x
Subject(s) - very long baseline interferometry , physics , ejecta , astrophysics , flare , astronomy , epoch (astronomy) , binary number , polarization (electrochemistry) , galaxy , supernova , chemistry , arithmetic , mathematics
We report the results of the first two 5‐GHz electronic very‐long‐baseline interferometry (e‐VLBI) observations of the X‐ray binary Cygnus X‐3 using the European VLBI Network. Two successful observing sessions were held, on 2006 April 20, when the system was in a quasi‐quiescent state several weeks after a major flare, and on 2006 May 18, a few days after another flare. At the first epoch we detected faint emission probably associated with a fading jet, spatially separated from the X‐ray binary. The second epoch in contrast reveals a bright, curved, relativistic jet more than 40 milliarcsec in extent. In the first and probably also second epochs the X‐ray binary core is not detected, which may indicate a temporary suppression of jet production as seen in some black hole X‐ray binaries in certain X‐ray states. Spatially resolved polarization maps at the second epoch provide evidence of interaction between the ejecta and the surrounding medium. These results clearly demonstrate the importance of rapid analysis of long‐baseline observations of transients, such as facilitated by e‐VLBI.