Possible Photometric Evidence of Ejection of Bullet Like Features in the Relativistic Jet source SS433

Details Possible Photometric Evidence of Ejection of Bullet Like Features in the Relativistic Jet source SS433 Possible Photometric Evidence of Ejection of Bullet Like Features in the Relativistic Jet source SS433

2004-02-24

arxiv.org/abs/astro-ph/0402560v1

Astrophys.J.595:L45,2003

Astronomy and Astrophysics

Astrophysics

9 latex pages with five figures

Scientific paper

10.1086/379003

SS433 is well-known for its precessing twin jets having optical bullets inferred through {\it spectroscopic} observation of $H_\alpha$ lines. Recently, Chakrabarti et al. (2002) described processes which may be operating in accretion disk of SS433 to produce these bullets. In a recent multi-wavelength campaign, we find sharp rise in intensity in time-scales of few minutes in X-rays, IR and radio waves through {\it photometric} studies. We interpret them to be possible evidence of ejection of bullet-like features from accretion disks.

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