Mass and spin measurements for the neutron star 4U1608−52 through the relativistic precession model-Reference-Cited by-同舟云学术

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Mass and spin measurements for the neutron star 4U1608−52 through the relativistic precession model

Published:2019-04-27 Issue:4 Volume:486 Page:4485-4497
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

du Buisson L¹,Motta S¹²^ORCID,Fender R¹³

Affiliation:

1. Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK

2. ESAC, European Space Astronomy Centre, Villanueva de la Cañada, E-28692 Madrid, Spain

3. Department of Astronomy, University of Cape Town, RW James Building, 9 University Avenue, Rondebosch 7701, South Africa

Funder

Science and Technology Facilities Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stz1160/28537833/stz1160.pdf

Reference74 articles.

1. A precise determination of black hole spin in GRO J1655-40

2. X‐Ray Time Variability Across the Atoll Source States of 4U 1636−53

3. LOW-FREQUENCY QUASI-PERIODIC OSCILLATION FROM THE 11 Hz ACCRETING PULSAR IN TERZAN 5: NOT FRAME DRAGGING

4. A Massive Pulsar in a Compact Relativistic Binary

5. An ultraluminous X-ray source powered by an accreting neutron star

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1. Black hole mass and spin measurements through the relativistic precession model: XTE J1859+226;Monthly Notices of the Royal Astronomical Society;2022-10-04

2. Realistic compact stars in conformal teleparallel gravity;Progress of Theoretical and Experimental Physics;2022-09

3. Simple Analytic Formula Relating the Mass and Spin of Accreting Compact Objects to Their Rapid X-Ray Variability;The Astrophysical Journal;2022-04-01

4. Very low-frequency oscillations from the 11 Hz pulsar in Terzan 5: frame dragging back on the table.;Monthly Notices of the Royal Astronomical Society;2021-02-12

5. A New Method to Constrain Neutron Star Structure from Quasi-periodic Oscillations;The Astrophysical Journal;2020-08-24

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