File(s) under permanent embargo
Consecutive bright pulses in the vela pulsar
journal contribution
posted on 2023-05-17, 09:48 authored by Jim PalfreymanJim Palfreyman, Hotan, AW, John DickeyJohn Dickey, Young, TG, Claire TrenhamWe report on the discovery of consecutive bright radio pulses from the Vela pulsar, a new phenomenon that may lead to a greater understanding of the pulsar emission mechanism. This results from a total of 345 hr worth of observations of the Vela pulsar using the University of Tasmania's 26 m radio telescope to study the frequency and statistics of abnormally bright pulses and sub-pulses. The bright pulses show a tendency to appear consecutively. The observations found two groups of six consecutive bright pulses and many groups of two to five bright pulses in a row. The strong radio emission process that produces the six bright pulses lasts between 0.4 and 0.6 s. The numbers of bright pulses in sequence far exceed what would be expected if individual bright pulses were independent random events. Consecutive bright pulses must be generated by an emission process that is long lived relative to the rotation period of the neutron star.
History
Publication title
The Astrophysical Journal LettersVolume
735Article number
L17Number
L17Pagination
1-3ISSN
2041-8205Department/School
School of Natural SciencesPublisher
Institute of Physics Publishing Ltd.Place of publication
United KingdomRights statement
Copyright 2011 The American Astronomical SocietyRepository Status
- Restricted