dc.contributor.author |
Chakrabarti, S. K |
|
dc.date.accessioned |
2006-03-14T09:12:45Z |
|
dc.date.available |
2006-03-14T09:12:45Z |
|
dc.date.issued |
2005-06 |
|
dc.identifier.citation |
BASI, Vol. 33, No. 2, pp. 109-115 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/759 |
|
dc.description.abstract |
We present a summary of the recent multiwavelength campaign made in September-October, 2002, to observe SS 433. We used the Giant Meterwave Radio Telescope (GMRT) for radio observation, 1.2 meter Physical Research Laboratory Infra-red telescope at Mt Abu for IR, 1 meter Telescope at the State Observatory, Nainital for Optical photometry, 2.3 meter optical telescope at the Vainu Bappu observatory for spectrum and Rossi X-ray Timing Explorer (RXTE) Target of Opportunity (TOO) for X-ray observations. Sharp variations in intensity in time-scales of a few minutes in X-rays, IR and radio wavelengths have been discovered. We also discover a delay of about two days between IR and Radio. Double Fe line pro les which corresponded to red and blue components of the relativistic jet have been found in X-ray data. We present the broadband spectrum averaged over the campaign duration |
en |
dc.format.extent |
195802 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.subject |
SS 433 - X-ray |
en |
dc.subject |
Infra-red and radio sources - stars |
en |
dc.title |
A recent multi-wavelength campaign to observe the microquasar SS433 |
en |
dc.type |
Article |
en |