dc.contributor.author |
Saha, S. K |
|
dc.contributor.author |
Maitra, D |
|
dc.date.accessioned |
2010-01-16T12:04:18Z |
|
dc.date.available |
2010-01-16T12:04:18Z |
|
dc.date.issued |
2001 |
|
dc.identifier.citation |
Indian Journal of Physics, Vol. 75B, pp. 391 - 398 |
en |
dc.identifier.issn |
1625-1776 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4984 |
|
dc.description.abstract |
Speckle interferometric technique is used to record a series of short exposure images of several close binary stars with sub-arcsecond separation through a narrow band filter centred at H$\alpha$ at the Cassegrain focus of the 2.34 meter Vainu Bappu telescope (VBT), situated at Vainu Bappu Observatory (VBO), Kavalur. The auto-correlation method is developed under Image Reduction Analysis Facility (IRAF). Wiener filter is included in the programme to eliminate spurious high frequency contributions; a few sets of data provide the optimised results. The auto-correlated image of these stars gives the separation of the binary components. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Indian Association for the Cultivation of Science |
en |
dc.relation.uri |
http://arxiv.org/abs/astro-ph/0106119 |
en |
dc.rights |
© Indian Association for the Cultivation of Science |
en |
dc.subject |
Speckle Imaging |
en |
dc.subject |
Auto-Correction |
en |
dc.subject |
Binary Stars |
en |
dc.title |
Auto-correlation of Binary stars |
en |
dc.type |
Article |
en |