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Though widely observed to be emanating out from a variety of galactic and
extra-galactic sources, the underlying physical mechanism behind the
formation of the Active Galactic Nuclei (AGN) and micro-quasar jets and outflows are
enshrouded by the veil of mystery till date. One of the most prominent signatures
of activities around the AGN
is the presence of mass outflows and
jets. AGNs produce cosmic jets through which immense amount of matter
and energy are ejected out of the cores of the galaxies.
Similarly, micro quasars have also been discovered where the mass
outflow is formed from stellar mass black hole candidates.
Possibly the sources of
ray bursts (GRB)
also suffer mass loss through jets and outflows.
Much work has been done
on how such jets interact with their surrounding and on how such interactions
may convey the informations about the morphology of different
Galactic and extra galactic sources. However,
the detailed nature
of the formation of such jets is not quite clear due to the
lack of proper understanding of the underlying physical mechanism
responsible for jet production. Neither the amount of matter
contained in these jets/outflows could accurately be calculated by any
definitive method.
From the theoretical front, the non stellar activities around the
above mentioned jet/outflow sources are thought to be produced by a powerful
engine, an accreting astrophysical black hole, sitting at their dynamical
centres. In this regard, it is also to be noted that since black holes
do not have their own `physical' atmosphere to contribute outgoing material,
jet/outflow for these candidates has to be generated from the
accreting material only. Hence, it is quite logical to conclude
that the jet formation from the above mentioned galactic and extra galactic sources,
and accretion onto their central black holes are not
two different issues to be studied disjointedly, rather they must be
strongly correlated and it is necessary to study the accretion and jet
within the same framework.
Next: Research Accomplished
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Tapas Kumar Das
2009-01-17