dc.contributor.author | Saraswat, P | |
dc.contributor.author | Apparao, K. M. V | |
dc.date.accessioned | 2008-07-11T10:21:46Z | |
dc.date.available | 2008-07-11T10:21:46Z | |
dc.date.issued | 1994 | |
dc.identifier.citation | IAU Symposium, No. 162, pp. 213 – 215 | en |
dc.identifier.issn | 0074-1809 | |
dc.identifier.uri | http://hdl.handle.net/2248/2638 | |
dc.format.extent | 293881 bytes | |
dc.format.mimetype | application/pdf | |
dc.language.iso | en | en |
dc.publisher | International Astronomical Union | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/1994IAUS..162..213S | en |
dc.subject | Star disk structure | en |
dc.subject | X-ray observations | en |
dc.subject | Stellar wind model | en |
dc.subject | 4U1907+09 | en |
dc.title | Be star disk structure as implied by X-ray observations | en |
dc.type | Article | en |