About: A 110-ms pulsar, with negative period derivative, in the globular cluster M15

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scientific article published in Nature

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rdf:type	Item
description	artículu científicu (ast) wetenschappelijk artikel (nl) article publié dans la revue scientifique Nature (fr) scientific article published in Nature (en) im Februar 1989 veröffentlichter wissenschaftlicher Artikel (de) наукова стаття, опублікована в Nature в лютому 1989 (uk)
publication date	wds:Q59071580-8C209B98-9B67-47D7-9589-0ED38057FBB0
publication date	1989-02-01 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q59071580-1029A923-65C7-4122-84CE-AE42FA9495B5
language of work or name	English
exact match	wds:Q59071580-97AB4DF7-2014-4384-9066-CD669E9C9375
exact match	https://scigraph.springernature.com/pub.10.1038/337531a0
cites work	wds:Q59071580-0053CB09-DD14-4921-87AD-B54F20D95B69 wds:Q59071580-0A0392A8-5CC2-4F6A-8F56-1E5F9833348C wds:Q59071580-58650F80-E85E-4E62-B296-36B685572967 wds:Q59071580-5BFE9BB2-9F17-497A-A1B0-0D31F6813EE6 wds:Q59071580-6D2C3FC7-89E9-424B-8C9D-67A32F0C24EF wds:Q59071580-6E0AED6E-DACD-4FB0-BEA9-A5452CE95695 wds:Q59071580-7BB59571-9F13-4141-B86C-3E931317F256 wds:Q59071580-842F8AB3-B171-4A4A-B865-426529C1BFDB wds:Q59071580-851BA611-58B3-4192-B848-F29E00C4A763 wds:Q59071580-8577065B-627E-4D8D-8691-E2E9CEC3D89D wds:Q59071580-88457F6A-73CD-4628-B293-BFB7061B87DC wds:Q59071580-AFB46075-A9C1-4336-A2BA-34F8882B1004 wds:Q59071580-B48598A4-62F3-4C01-9AEE-63B180426CB5 wds:Q59071580-B706EEEF-B1B1-4DB9-A9B3-7E1B39B4E78C wds:Q59071580-BD6F00D4-AEAF-4F81-92F3-B3B585B6376E wds:Q59071580-CC25711E-7601-49BC-B6CD-C0E3B63492B3 wds:Q59071580-EA7CCA09-EFB7-4B88-8A1B-B780D3B45F49
cites work	Ablating dwarf model for eclipsing millisecond pulsar 1957 + 20 The galactic population of pulsars Nature and evolution of the eclipsing millisecond binary pulsar PSR1957 + 20 Fate of the companion stars of ultra-rapid pulsars Formation of a millisecond pulsar in a globular cluster Formation of isolated millisecond pulsars in globular clusters The discovery of a millisecond pulsar in the globular cluster M28 A millisecond pulsar in an eclipsing binary Optical identification of binary pulsars - Implications for magnetic field decay in neutron stars A new class of radio pulsars The spin histories of PSR1821 –24 in M28 and PSR1951 + 32 in CTB80 Discovery of a binary millisecond pulsar in the globular cluster M4 Period derivative of the millisecond pulsar in globular cluster M 28 Mass transfer instabilities due to angular momentum flows in close binaries Accurate optical positions for the centers of galactic globular clusters Arrival-time analysis for a millisecond pulsar The structure of stars. VI. Observed radii and structural parameters in globular clusters
author name string	wds:Q59071580-43262C72-4B8F-4286-A901-674CBF4BF3EB wds:Q59071580-57CBA1CC-728D-4F3C-913C-86D6800F1396 wds:Q59071580-6ED130D0-47ED-489B-ACF7-C25EE76BF39E wds:Q59071580-906C5B0D-FDE6-4106-A0EB-435A477F01D8 wds:Q59071580-B946CC4A-6CE6-4CB9-90E7-0D8B8FD20594 wds:Q59071580-E3C2B360-3E2F-4DAE-BAF6-B231D56BA459
author name string	S. R. Kulkarni A. S. Fruchter A. Wolszczan D. C. Backer J. Middleditch R. J. Dewey
rdfs:label	A 110-ms pulsar, with negative period derivative, in the globular cluster M15 (en) A 110-ms pulsar, with negative period derivative, in the globular cluster M15 (nl)
skos:prefLabel	A 110-ms pulsar, with negative period derivative, in the globular cluster M15 (en) A 110-ms pulsar, with negative period derivative, in the globular cluster M15 (nl)
name	A 110-ms pulsar, with negative period derivative, in the globular cluster M15 (en) A 110-ms pulsar, with negative period derivative, in the globular cluster M15 (nl)
title	wds:Q59071580-53EE1058-3828-41C2-AA4A-B07FCE85044F
title	A 110-ms pulsar, with negative period derivative, in the globular cluster M15 (en)
page(s)	wds:Q59071580-8F218A3D-A8BF-4A84-B582-DBCF3543523A
page(s)	531–533
instance of	wds:Q59071580-BE5DCEF5-85AF-4F78-B7CB-DA9DEA2303CB
instance of	scholarly article
published in	wds:Q59071580-40704A99-DE5D-4E42-8DB3-3113F6ABD0A9
published in	Nature
issue	wds:Q59071580-4993416C-C60B-4B73-BDC2-78DE16936336
volume	wds:Q59071580-D5BD8AFE-0311-4FA7-9101-99DC538DCCE2
issue	6207
volume	337
DOI	wds:Q59071580-3E1AF3D2-4FA9-47DA-890C-A6BE3BD9599E
DOI	http://dx.doi.org/10.1038/337531A0
DOI	10.1038/337531A0
ADS bibcode	wds:Q59071580-EE7B05EF-931C-4CDA-A393-EE0BDE4AA858
ADS bibcode	1989Natur.337..531W
Dimensions Publication ID	wds:Q59071580-E0B254C9-E6D1-47F1-AC51-CB2D64510DD6
Dimensions Publication ID	1031388349
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q59071580
is cites work of	Evacuation of gas from globular clusters by winds from millisecond pulsars Discovery of ten millisecond pulsars in the globular cluster 47 Tucanae Electromagnetic transients as triggers in searches for gravitational waves from compact binary mergers A nearby 37.9-ms radio pulsar in a relativistic binary system Spin-up more apparent than real Good things come in threes Discovery of two radio pulsars in the globular cluster M15 Binary and Millisecond Pulsars at the New Millennium Old pulsars in the low-density globular clusters MI3 and M53 Effect of small interpulsar distances in stochastic gravitational wave background searches with pulsar timing arrays Finding pulsars at Parkes Genesis of pulsars in globular clusters
is cites work of	wds:Q57407217-6E2421A2-173E-4489-94DB-AF155B8AA4B2 wds:Q59000025-1A145E14-2C8F-4133-9F9C-99EC0FA55166 wds:Q59008502-D2B49C2B-5854-4CBB-8FA7-814486E406EE

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