What is special about HBRPs
| dc.creator | Vranesevic, N. | |
| dc.creator | Melrose, D. B. | |
| dc.creator | Manchester, R. N. | |
| dc.date | 2006-04-18 | |
| dc.date.accessioned | 2026-07-07T07:04:40Z | |
| dc.date.available | 2026-07-07T07:04:40Z | |
| dc.description | The Parkes Multibeam Survey led to the identification ofa number of long-period radio pulsars with magnetic field well above the quantum critical field of 4.4 times 10 to 13 G (defined as high magnetic field radio pulsars - HBRPs). Traditional pulsar emission theories postulate that radio emission is suppressed above this critical field. The aim of thisproject is to understand emission properties of HBRPs. | |
| dc.description | 6 pages, 5 figures, in press ChJAA | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0604368 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0604368 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/109402 | |
| dc.subject | Astrophysics | |
| dc.title | What is special about HBRPs | |
| dc.type | text |