dc.contributor.author |
Joshi, U. C |
|
dc.contributor.author |
Chauhan, J. S |
|
dc.contributor.author |
Deshpande, M. R |
|
dc.contributor.author |
Sen, A. K |
|
dc.contributor.author |
Bhatnagar, A. K |
|
dc.date.accessioned |
2007-05-10T08:51:52Z |
|
dc.date.available |
2007-05-10T08:51:52Z |
|
dc.date.issued |
1993 |
|
dc.identifier.citation |
BASI, Vol. 21, pp. 651-653 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/1577 |
|
dc.description.abstract |
Comet Austin (1989c) was observed during April and May 1990 when its phase was between 106 deg and 110 deg. No unusual activity in the form of jet is seen in the polarization map. Polarization is low near the nucleus and high (approximately 16%) in the outer region (mean distance of 190,000 km on west side), suggesting segregation of grains |
en |
dc.format.extent |
423877 bytes |
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dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.subject |
Comet |
en |
dc.subject |
Polarimetry |
en |
dc.title |
Imaging polarimetry of comet Austin |
en |
dc.type |
Article |
en |