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On the timing history of PSR B1509 – 58

Blandford, R. D. (1994) On the timing history of PSR B1509 – 58. Monthly Notices of the Royal Astronomical Society, 267 (1). L7-L8. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20190523-125439160

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Abstract

The measurement of the third frequency derivative of PSR B1509–58 reported by Kaspi et al. is consistent with a constant magnetic moment. If a more accurate, stable measurement can be made, it should be possible to test directly models in which the magnetic moment varies.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/267.1.l7DOIArticle
http://adsabs.harvard.edu/abs/1994MNRAS.267L...7BADSArticle
ORCID:
AuthorORCID
Blandford, R. D.0000-0002-1854-5506
Additional Information:© 1994 Royal Astronomical Society. Provided by the NASA Astrophysics Data System. Accepted 1994 January 3. Received 1993 December 13. I thank Curtis Michel for bringing this observation to my attention and Vicky Kaspi and Steve Thorsett for constructive comments on the manuscript. Support under NSF contract AST 93-23370 and NASA contract NAGW2372 is gratefully acknowledged.
Group:TAPIR
Funders:
Funding AgencyGrant Number
NSFAST 93-23370
NASANAGW 2372
Subject Keywords:MHD, stars: magnetic fields, pulsars: general, pulsars: individual: B1509 – 58
Issue or Number:1
Record Number:CaltechAUTHORS:20190523-125439160
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190523-125439160
Official Citation:R. D. Blandford, On the timing history of PSR B1509 – 58, Monthly Notices of the Royal Astronomical Society, Volume 267, Issue 1, 1 March 1994, Pages L7–L8, https://doi.org/10.1093/mnras/267.1.L7
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:95753
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:24 May 2019 16:59
Last Modified:03 Oct 2019 21:16

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