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dc.contributor.author
Bult, Peter  
dc.contributor.author
Altamirano, Diego  
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Arzoumanian, Zaven  
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Chakrabarty, Kuheli  
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Chenevez, Jérôme  
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Ferrara, Elizabeth C.  
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Gendreau, Keith C.  
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Guillot, Sebastien  
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Güver, Tolga  
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Iwakiri, Wataru  
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Jaisawal, Gaurava K.  
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Mancuso, Giulio Cesare  
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Malacaria, Christian  
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Ng, Mason  
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Sanna, Andrea  
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Strohmayer, Tod E.  
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Wadiasingh, Zorawar  
dc.contributor.author
Wolff, Michael T.  
dc.date.available
2023-07-13T16:11:01Z  
dc.date.issued
2022-08  
dc.identifier.citation
Bult, Peter; Altamirano, Diego; Arzoumanian, Zaven; Chakrabarty, Kuheli; Chenevez, Jérôme; et al.; The Discovery of the 528.6 Hz Accreting Millisecond X-Ray Pulsar MAXI J1816-195; IOP Publishing; The Astrophysical Journal Letters; 935; 2; 8-2022; 1-6  
dc.identifier.issn
2041-8205  
dc.identifier.uri
http://hdl.handle.net/11336/203812  
dc.description.abstract
We present the discovery of 528.6 Hz pulsations in the new X-ray transient MAXI J1816-195. Using NICER, we observed the first recorded transient outburst from the neutron star low-mass X-ray binary MAXI J1816-195 over a period of 28 days. From a timing analysis of the 528.6 Hz pulsations, we find that the binary system is well described as a circular orbit with an orbital period of 4.8 hr and a projected semimajor axis of 0.26 lt-s for the pulsar, which constrains the mass of the donor star to 0.10-0.55 M ⊙. Additionally, we observed 15 thermonuclear X-ray bursts showing a gradual evolution in morphology over time, and a recurrence time as short as 1.4 hr. We did not detect evidence for photospheric radius expansion, placing an upper limit on the source distance of 8.6 kpc.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
IOP Publishing  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Low mass X-ray binaries  
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Millisecond pulsars  
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X-ray bursts  
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Astronomía  
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Ciencias Físicas  
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CIENCIAS NATURALES Y EXACTAS  
dc.title
The Discovery of the 528.6 Hz Accreting Millisecond X-Ray Pulsar MAXI J1816-195  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2023-06-29T17:53:56Z  
dc.identifier.eissn
2041-8213  
dc.journal.volume
935  
dc.journal.number
2  
dc.journal.pagination
1-6  
dc.journal.pais
Reino Unido  
dc.description.fil
Fil: Bult, Peter. Department Of Astronomy, University Of Maryland; Estados Unidos  
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Fil: Altamirano, Diego. University of Southampton; Reino Unido  
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Fil: Arzoumanian, Zaven. Nasa Goddard Space Flight Center; Estados Unidos  
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Fil: Chakrabarty, Kuheli. Mit Kavli Institute For Astrophysics And Space Research; Estados Unidos  
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Fil: Chenevez, Jérôme. Technical University of Denmark; Dinamarca  
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Fil: Ferrara, Elizabeth C.. Department Of Astronomy, University Of Maryland; Estados Unidos  
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Fil: Gendreau, Keith C.. Nasa Goddard Space Flight Center; Estados Unidos  
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Fil: Guillot, Sebastien. Institut de Recherche En Astrophysique Et Planétologie; Francia  
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Fil: Güver, Tolga. Istanbul University; Turquía  
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Fil: Iwakiri, Wataru. Chuo University; Japón  
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Fil: Jaisawal, Gaurava K.. Technical University of Denmark; Dinamarca  
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Fil: Mancuso, Giulio Cesare. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina  
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Fil: Malacaria, Christian. International Space Science Institute; Suiza  
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Fil: Ng, Mason. Mit Kavli Institute For Astrophysics And Space Research; Estados Unidos  
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Fil: Sanna, Andrea. Università Degli Studi Di Cagliari.; Italia  
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Fil: Strohmayer, Tod E.. Nasa Goddard Space Flight Center; Estados Unidos  
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Fil: Wadiasingh, Zorawar. Department Of Astronomy, University Of Maryland; Estados Unidos  
dc.description.fil
Fil: Wolff, Michael T.. Spece Sciences División. Naval Research Laboratory; Estados Unidos  
dc.journal.title
The Astrophysical Journal Letters  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/2041-8213/ac87f9  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.3847/2041-8213/ac87f9