C H A N D R A
S C I E N C E
C E N T E R O B S E R V A T I O N C A T A L O G |
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Abstract: The X-ray binary SS 433, a Galactic microquasar, has been hypothesized to be an ultraluminous X-ray source (ULX) like those observed in nearby galaxies. It is well known that the compact object emits oppositely directed semi-relativistic jets that carry a much larger kinetic power than observed radiatively in the X-ray band. Much of the radiative power may be obscured from our view, which would link SS 433 to ULXs. SS 433 has extended X-ray emission, like Sy 2s where the extended gas is photo-excited by the obscured nuclear X-ray emission. We propose to test the model that SS 433's extended X-ray emission is reflected core emission by tracking the variability of the arc-second scale extended emission and testing for the expected correlation with the core flux. |
Remarks: Swift observations should be carried out every 3 +/- 1 days at 1 ks each starting at least 80 days before the first of the HRC observations and extending throughout the Chandra campaign. |
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