A Search for Giant Pulses from Millisecond Pulsars

We have searched for microsecond-timescale broadband emission from a sample of 18 millisecond pulsars. Our study places strong limits on such emission from several millisecond pulsars and shows that it is only present in a small subset of millisecond pulsars. Giant pulses of up to 64 times the mean...

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Main Authors: Knight, H., Bailes, M., Manchester, R., Ord, Stephen
Format: Journal Article
Published: Institute of Physics Publishing, Inc. 2005
Subjects:
Online Access:http://hdl.handle.net/20.500.11937/24278
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author Knight, H.
Bailes, M.
Manchester, R.
Ord, Stephen
author_facet Knight, H.
Bailes, M.
Manchester, R.
Ord, Stephen
author_sort Knight, H.
building Curtin Institutional Repository
collection Online Access
description We have searched for microsecond-timescale broadband emission from a sample of 18 millisecond pulsars. Our study places strong limits on such emission from several millisecond pulsars and shows that it is only present in a small subset of millisecond pulsars. Giant pulses of up to 64 times the mean pulse energy were detected from PSR J1823-3021A in the globular cluster NGC 6624. In contrast to the giant pulses of PSR B1937+21, nearly all of the giant pulses from PSR J1823-3021A were distributed within the trailing half of the main-pulse component of the integrated pulse profile. The fact that no giant pulses were observed on the leading side of the main-pulse component suggests that giant pulses are preferentially emitted closer to the last open field line than ordinary emission. The correlation between giant pulse emissivity and spin-down luminosity in millisecond pulsars suggests that the high period derivative of PSR J1823-3021A is intrinsic and is not just an artifact of its acceleration in the gravitational potential of NGC 6624.
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spelling curtin-20.500.11937-242782017-09-13T15:08:55Z A Search for Giant Pulses from Millisecond Pulsars Knight, H. Bailes, M. Manchester, R. Ord, Stephen Stars: Pulsars: Individual: Alphanumeric: PSR J1823-3021A Stars: Pulsars: General We have searched for microsecond-timescale broadband emission from a sample of 18 millisecond pulsars. Our study places strong limits on such emission from several millisecond pulsars and shows that it is only present in a small subset of millisecond pulsars. Giant pulses of up to 64 times the mean pulse energy were detected from PSR J1823-3021A in the globular cluster NGC 6624. In contrast to the giant pulses of PSR B1937+21, nearly all of the giant pulses from PSR J1823-3021A were distributed within the trailing half of the main-pulse component of the integrated pulse profile. The fact that no giant pulses were observed on the leading side of the main-pulse component suggests that giant pulses are preferentially emitted closer to the last open field line than ordinary emission. The correlation between giant pulse emissivity and spin-down luminosity in millisecond pulsars suggests that the high period derivative of PSR J1823-3021A is intrinsic and is not just an artifact of its acceleration in the gravitational potential of NGC 6624. 2005 Journal Article http://hdl.handle.net/20.500.11937/24278 10.1086/429533 Institute of Physics Publishing, Inc. unknown
spellingShingle Stars: Pulsars: Individual: Alphanumeric: PSR J1823-3021A
Stars: Pulsars: General
Knight, H.
Bailes, M.
Manchester, R.
Ord, Stephen
A Search for Giant Pulses from Millisecond Pulsars
title A Search for Giant Pulses from Millisecond Pulsars
title_full A Search for Giant Pulses from Millisecond Pulsars
title_fullStr A Search for Giant Pulses from Millisecond Pulsars
title_full_unstemmed A Search for Giant Pulses from Millisecond Pulsars
title_short A Search for Giant Pulses from Millisecond Pulsars
title_sort search for giant pulses from millisecond pulsars
topic Stars: Pulsars: Individual: Alphanumeric: PSR J1823-3021A
Stars: Pulsars: General
url http://hdl.handle.net/20.500.11937/24278