Please use this identifier to cite or link to this item:
http://hdl.handle.net/2289/1385
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Kapoor, R.C. | - |
dc.contributor.author | Shukre, C.S. | - |
dc.date.accessioned | 2006-06-27T07:31:18Z | - |
dc.date.available | 2006-06-27T07:31:18Z | - |
dc.date.issued | 2002 | - |
dc.identifier.citation | Bulletin of the Astronomical Society of India, 2002, Vol.30, p695-696 | en |
dc.identifier.issn | 0304-9523 | - |
dc.identifier.uri | http://hdl.handle.net/2289/1385 | - |
dc.description | Presented at the 21st meeting of the Astronomical Society of India, Pune, 2002. | en |
dc.description.abstract | By attributing the often seen longitude offsets between the core and conal component centres of pulsar radio pulses to different emission altitudes, we present a new method for investigating these altitudes. Our method can explain these offsets and also sheds light on them. | en |
dc.format.extent | 52426 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | The Astronomical Society of India | en |
dc.rights | (2002) by the Astronomical Society of India. | en |
dc.title | Radio pulsar emission altitudes | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
2002 BASI V30 p695-696.pdf | 2p. | 51.2 kB | Adobe PDF | View/Open |
Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.