Please use this identifier to cite or link to this item:
http://hdl.handle.net/2289/1541
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Nelemans, G. | - |
dc.contributor.author | Hartman, J.W. | - |
dc.contributor.author | Verbunt, F. | - |
dc.contributor.author | Bhattacharya, D. | - |
dc.contributor.author | Wijers, R.A.M.J. | - |
dc.date.accessioned | 2006-11-24T11:18:43Z | - |
dc.date.available | 2006-11-24T11:18:43Z | - |
dc.date.issued | 1997-06 | - |
dc.identifier.citation | Astronomy and Astrophysics, 1997, Vol.322, p489-492 | en |
dc.identifier.issn | 0004-6361 | - |
dc.identifier.uri | http://hdl.handle.net/2289/1541 | - |
dc.description.abstract | On the basis of a highly simplified model for small scale structure in the electron density distribution in the Galaxy, we argue that the spread of expectation values for the dispersion measure at given distance is proportional to the square root of the dispersion measure as found from a smooth model for the electron distribution. We show that this simple method leads to appreciable improvement in the description of dispersion measures in a full population synthesis. | en |
dc.format.extent | 326894 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Springer-Verlag | en |
dc.relation.uri | http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997A%26A...322..489N&link_type=ARTICLE&db_key=AST | en |
dc.rights | (1997) by European Southern Observatory | en |
dc.subject | PULSARS: GENERAL, | en |
dc.subject | ISM: STRUCTURE | en |
dc.title | Modelling the variance of dispersion measures of radio pulsars. | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1997 AA V322 p489.pdf | 319.23 kB | Adobe PDF | View/Open |
Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.