The case for no field decay from improved pulsar population studies
| dc.contributor.author | Hartman, J W | |
| dc.contributor.author | Verbunt, F | |
| dc.contributor.author | Bhattacharya, D | |
| dc.contributor.author | Wijers, H | |
| dc.date.accessioned | 2007-05-25T08:40:54Z | |
| dc.date.available | 2007-05-25T08:40:54Z | |
| dc.date.issued | 1996 | |
| dc.description | Open Access. Pulsars: problems and progressAstronomical Society of the Pacific Conference Series, Vol. 105; Proceedings of the 160th colloquium of the International Astronomical Union held in Sydney; Australia; 8-12 January 1996; San Francisco: Astronomical Society of the Pacific (ASP); 1996; edited by S. Johnston, M.A. Walker, and M. Bailes. | en |
| dc.format.extent | 161554 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.citation | IAU Colloquium, 1996, Vol.160, p47 | en |
| dc.identifier.uri | http://hdl.handle.net/2289/2423 | |
| dc.language.iso | en | en |
| dc.publisher | Astronomical Society of Pacific | en |
| dc.relation.uri | http://adsabs.harvard.edu/cgi-bin/bib_query?1996ASPC..105...47H | en |
| dc.rights | 1996 Astronomical Society of the Pacific | en |
| dc.title | The case for no field decay from improved pulsar population studies | en |
| dc.type | Article | en |