dc.contributor.author |
Kharb, P |
|
dc.contributor.author |
Gabuzda, D |
|
dc.contributor.author |
Shastri, P |
|
dc.date.accessioned |
2008-06-25T10:33:13Z |
|
dc.date.available |
2008-06-25T10:33:13Z |
|
dc.date.issued |
2003 |
|
dc.identifier.citation |
BASI, Vol. 31, No. 3&4, pp. 433 - 435 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2505 |
|
dc.description.abstract |
Multi-epoch Very Long Baseline Polarimetric observations of the Broad Line Radio galaxy 3C111 performed at 8 and 43 GHz after a large millimetre outburst, reveal rapidly evolving parsec-scale radioo structure and the corresponding evolution of the magnetic field geometry. |
en |
dc.format.extent |
89899 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.relation.uri |
http://adsabs.harvard.edu/abs/2003BASI...31..433K |
en |
dc.subject |
Magnetic field |
en |
dc.subject |
Polarization |
en |
dc.title |
Magnetic Field Geometry of 3C111 on pc-scales |
en |
dc.type |
Article |
en |