Turn-over in pulsar spectra above 1 GHz

Simple item page
dc.creatorKijak, J.
dc.creatorGupta, Y.
dc.creatorKrzeszowski, K.
dc.date2007-01-09
dc.date.accessioned2026-07-07T07:39:16Z
dc.date.available2026-07-07T07:39:16Z
dc.descriptionWe present the first direct evidence for turn-over in pulsar radio spectra at high frequencies. Two pulsars are now shown to have a turn-over frequency > 1GHz. We also find some evidence that the peak frequency of turn-over in pulsar spectra appears to depend on dispersion measure and pulsar age.
dc.descriptionProceedings of the 363. WE-Heraeus Seminar on: Neutron Stars and Pulsars (Posters and contributed talks) Physikzentrum Bad Honnef, Germany, May.14-19, 2006, eds. W.Becker, H.H.Huang, MPE Report 291, pp.84-87
dc.identifierhttps://arxiv.org/abs/astro-ph/0701223
dc.identifierhttp://arxiv.org/abs/astro-ph/0701223
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/121385
dc.subjectAstrophysics
dc.titleTurn-over in pulsar spectra above 1 GHz
dc.typetext

Files

Collections

arXiv