dc.contributor.author |
Roy, S |
|
dc.date.accessioned |
2008-07-18T07:22:12Z |
|
dc.date.available |
2008-07-18T07:22:12Z |
|
dc.date.issued |
2002-09 |
|
dc.identifier.citation |
BASI, Vol. 30, No. 3, pp. 637 - 642 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2746 |
|
dc.description.abstract |
The central region of our milky way Galaxy still eludes a comprehensive
understanding. With new observations. however. we are being able to know many
of the observable properties of the sources, which allow us to better understand the
actual physical processes operating in the region. Here, we discuss about the present
status and the new observations in the radio wavelengths to constrain the source
properties in this complex region. |
en |
dc.format.extent |
193386 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.subject |
Galactic Centre Environment |
en |
dc.subject |
Interstellar Medium |
en |
dc.subject |
GC Filamentary Structures |
en |
dc.subject |
Galactic Longitude |
en |
dc.title |
Radio study of the Galactic Centre Environment |
en |
dc.type |
Article |
en |