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Article: Remarks on triaxiality, spin-up, and magnetic field obliquity of some millisecond pulsars

TitleRemarks on triaxiality, spin-up, and magnetic field obliquity of some millisecond pulsars
Authors
Chau, WYCheng, KSZhang, JL
KeywordsPulsars: General
Stars: Neutron
Stars: Rotation
Issue Date1992
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205
Citation
Astrophysical Journal Letters, 1992, v. 390 n. 2, p. 486-488 How to Cite?
AbstractWe show how two "observed" properties of millisecond pulsars - a very small nonaxisymmetry in the mass distribution and the near-orthogonality between the rotational and the magnetic axis - can find very natural explanation within the context of the collapse formation and evolution of such objects modeled by uniform density ellipsoids. This could also provide alternate explanations to the observed spin-up of some pulsars in globular clusters.
Persistent Identifierhttp://hdl.handle.net/10722/174905
ISSN
2041-8205
2022 Impact Factor: 7.9
2020 SCImago Journal Rankings: 3.639
ISI Accession Number ID
WOS:A1992HR23200018

 

DC FieldValueLanguage
dc.contributor.authorChau, WYen_US
dc.contributor.authorCheng, KSen_US
dc.contributor.authorZhang, JLen_US
dc.date.accessioned2012-11-26T08:48:03Z-
dc.date.available2012-11-26T08:48:03Z-
dc.date.issued1992en_US
dc.identifier.citationAstrophysical Journal Letters, 1992, v. 390 n. 2, p. 486-488en_US
dc.identifier.issn2041-8205en_US
dc.identifier.urihttp://hdl.handle.net/10722/174905-
dc.description.abstractWe show how two "observed" properties of millisecond pulsars - a very small nonaxisymmetry in the mass distribution and the near-orthogonality between the rotational and the magnetic axis - can find very natural explanation within the context of the collapse formation and evolution of such objects modeled by uniform density ellipsoids. This could also provide alternate explanations to the observed spin-up of some pulsars in globular clusters.en_US
dc.languageengen_US
dc.publisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205en_US
dc.relation.ispartofAstrophysical Journal Lettersen_US
dc.subjectPulsars: Generalen_US
dc.subjectStars: Neutronen_US
dc.subjectStars: Rotationen_US
dc.titleRemarks on triaxiality, spin-up, and magnetic field obliquity of some millisecond pulsarsen_US
dc.typeArticleen_US
dc.identifier.emailCheng, KS: hrspksc@hkucc.hku.hken_US
dc.identifier.authorityCheng, KS=rp00675en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.scopuseid_2-s2.0-11944271982en_US
dc.identifier.volume390en_US
dc.identifier.issue2en_US
dc.identifier.spage486en_US
dc.identifier.epage488en_US
dc.identifier.isiWOS:A1992HR23200018-
dc.publisher.placeUnited Kingdomen_US
dc.identifier.scopusauthoridChau, WY=7006157958en_US
dc.identifier.scopusauthoridCheng, KS=9745798500en_US
dc.identifier.scopusauthoridZhang, JL=14039783200en_US
dc.identifier.issnl2041-8205-

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