Simultaneous radio and X-ray observations of the transitional millisecond pulsar candidate 3FGL J1544.6-1125
All data analysed in this article are public. The VLA data can be downloaded from the National Radio Astronomy Observatory (NRAO) Data Archive (https://data.nrao.edu) under project code VLA 18A-398. The Chandra data can be downloaded from the Chandra Data Archive (https://cda.harvard.edu/chaser/) us...
| Autores: | , , , , , , , , |
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| Tipo de documento: | artigo |
| Estado: | Versão publicada |
| Data de publicação: | 2025 |
| País: | España |
| Recursos: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositório: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
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| Acesso em linha: | http://hdl.handle.net/10261/427630 https://api.elsevier.com/content/abstract/scopus_id/105033457174 |
| Access Level: | Acceso aberto |
| Palavra-chave: | Radio continuum: transients Stars: neutron X-rays: binaries |
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Simultaneous radio and X-ray observations of the transitional millisecond pulsar candidate 3FGL J1544.6-1125 |
| title |
Simultaneous radio and X-ray observations of the transitional millisecond pulsar candidate 3FGL J1544.6-1125 |
| spellingShingle |
Simultaneous radio and X-ray observations of the transitional millisecond pulsar candidate 3FGL J1544.6-1125 Gusinskaia, Nina V. Radio continuum: transients Stars: neutron X-rays: binaries |
| title_short |
Simultaneous radio and X-ray observations of the transitional millisecond pulsar candidate 3FGL J1544.6-1125 |
| title_full |
Simultaneous radio and X-ray observations of the transitional millisecond pulsar candidate 3FGL J1544.6-1125 |
| title_fullStr |
Simultaneous radio and X-ray observations of the transitional millisecond pulsar candidate 3FGL J1544.6-1125 |
| title_full_unstemmed |
Simultaneous radio and X-ray observations of the transitional millisecond pulsar candidate 3FGL J1544.6-1125 |
| title_sort |
Simultaneous radio and X-ray observations of the transitional millisecond pulsar candidate 3FGL J1544.6-1125 |
| dc.creator.none.fl_str_mv |
Gusinskaia, Nina V. Jaodand, Amruta D. Hessels, Jason W. T. Bogdanov, Slavko Deller, Adam T. Miller-Jones, J. C. A. Russell, T. D. Patruno, Alessandro Archibald, Anne M. |
| author |
Gusinskaia, Nina V. |
| author_facet |
Gusinskaia, Nina V. Jaodand, Amruta D. Hessels, Jason W. T. Bogdanov, Slavko Deller, Adam T. Miller-Jones, J. C. A. Russell, T. D. Patruno, Alessandro Archibald, Anne M. |
| author_role |
author |
| author2 |
Jaodand, Amruta D. Hessels, Jason W. T. Bogdanov, Slavko Deller, Adam T. Miller-Jones, J. C. A. Russell, T. D. Patruno, Alessandro Archibald, Anne M. |
| author2_role |
author author author author author author author author |
| dc.contributor.none.fl_str_mv |
NASA University of Toronto Netherlands Research School for Astronomy Natural Sciences and Engineering Research Council of Canada Ministerio de Ciencia, Innovación y Universidades (España) Agencia Estatal de Investigación (España) Generalitat de Catalunya The Dunlap Family Patruno, Alessandro [0000-0002-6459-0674] Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| dc.subject.none.fl_str_mv |
Radio continuum: transients Stars: neutron X-rays: binaries |
| topic |
Radio continuum: transients Stars: neutron X-rays: binaries |
| description |
All data analysed in this article are public. The VLA data can be downloaded from the National Radio Astronomy Observatory (NRAO) Data Archive (https://data.nrao.edu) under project code VLA 18A-398. The Chandra data can be downloaded from the Chandra Data Archive (https://cda.harvard.edu/chaser/) using observation IDs 20902 and 20903, as well as the HEASARC archive (https://heasarc.gsfc.nasa.gov/docs/archive.html). The derived data generated in this research will be shared on reasonable request to the corresponding author. |
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2025 |
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2025 2026 2026 |
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info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion |
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article |
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http://hdl.handle.net/10261/427630 https://api.elsevier.com/content/abstract/scopus_id/105033457174 |
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http://hdl.handle.net/10261/427630 https://api.elsevier.com/content/abstract/scopus_id/105033457174 |
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Inglés |
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Inglés |
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#PLACEHOLDER_PARENT_METADATA_VALUE# info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-124581OB-I00 The underlying dataset has been published as supplementary material of the article in the publisher platform at DOI 10.1093/mnras/stae2577 https://doi.org/10.1093/mnras/stae2577 Sí |
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info:eu-repo/semantics/openAccess |
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openAccess |
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application/pdf |
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Oxford University Press Royal Astronomical Society |
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Oxford University Press Royal Astronomical Society |
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reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC) |
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Simultaneous radio and X-ray observations of the transitional millisecond pulsar candidate 3FGL J1544.6-1125Gusinskaia, Nina V.Jaodand, Amruta D.Hessels, Jason W. T.Bogdanov, SlavkoDeller, Adam T.Miller-Jones, J. C. A.Russell, T. D.Patruno, AlessandroArchibald, Anne M.Radio continuum: transientsStars: neutronX-rays: binariesAll data analysed in this article are public. The VLA data can be downloaded from the National Radio Astronomy Observatory (NRAO) Data Archive (https://data.nrao.edu) under project code VLA 18A-398. The Chandra data can be downloaded from the Chandra Data Archive (https://cda.harvard.edu/chaser/) using observation IDs 20902 and 20903, as well as the HEASARC archive (https://heasarc.gsfc.nasa.gov/docs/archive.html). The derived data generated in this research will be shared on reasonable request to the corresponding author.Transitional millisecond pulsars (tMSPs) are neutron star systems that alternate between a rotation-powered radio millisecond pulsar state and an accretion disc-dominated low-mass X-ray binary (LMXB)-like state on multi-year time-scales. During the LMXB-like state, the X-ray emission from tMSPs switches between 'low' and 'high' X-ray brightness modes on a time-scale of seconds to minutes (or longer), while the radio emission shows variability on time-scales of roughly minutes. Coordinated Very Large Array (VLA) and Chandra observations of the nearby tMSP PSR J1023+0038 uncovered a clear anticorrelation between radio and X-ray luminosities such that the radio emission consistently peaks during the X-ray low modes. In addition, there are sometimes also radio/X-ray flares that show no obvious correlation. In this paper, we present simultaneous radio and X-ray observations of a promising tMSP candidate system, 3FGL J1544.61125, which shows optical, -ray, and X-ray phenomena similar to PSR J1023+0038, but which is challenging to study because of its greater distance. Using simultaneous VLA and Chandra observations, we find that the radio and X-ray emission are consistent with being anticorrelated in a manner similar to PSR J1023+0038. We discuss how our results help in understanding the origin of bright radio emission from tMSPs. The greater sensitivity of upcoming telescopes such as the Square Kilometre Array will be crucial for studying the correlated radio/X-ray phenomena of tMSP systems.The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. The scientific results reported in this article are based in part on observations made by the Chandra X-ray Observatory, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of NASA under contract NAS8-03060. This research has relied on software provided by the Chandra X-ray Center (CXC) in the application packages ciao and software provided by the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC and the High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory. We acknowledge extensive use of NASA’s Astrophysics Data System Bibliographic Services and arXiv. The Dunlap Institute is funded through an endowment established by the David Dunlap family and the University of Toronto. NVG acknowledges partial funding from Nederlandse Onderzoekschool Voor Astronomie (NOVA) and the Natural Sciences and Engineering Research Council of Canada (NSERC). AP was partially supported by the grant PID2021-124581OB-I00 funded by MCIU/AEI and 2021SGR00426 of the Generalitat de Catalunya. ADJ was partially supported by the Chandra X-ray Center Award No. GO0-21067X.Peer reviewedOxford University PressRoyal Astronomical SocietyNASAUniversity of TorontoNetherlands Research School for AstronomyNatural Sciences and Engineering Research Council of CanadaMinisterio de Ciencia, Innovación y Universidades (España)Agencia Estatal de Investigación (España)Generalitat de CatalunyaThe Dunlap FamilyPatruno, Alessandro [0000-0002-6459-0674]Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202620262025info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/427630https://api.elsevier.com/content/abstract/scopus_id/105033457174reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-124581OB-I00The underlying dataset has been published as supplementary material of the article in the publisher platform at DOI 10.1093/mnras/stae2577https://doi.org/10.1093/mnras/stae2577Síinfo:eu-repo/semantics/openAccessoai:dnet:digitalcsic_::83465210eeadc7f08d0ac676ad59b3d72026-05-22T06:33:51Z |
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