The DOI matches its Crossref record; 28 of the 28 references it cites were found in a registry or an index.
THE DISTANCE, MASS, AND RADIUS OF THE NEUTRON STAR IN 4U 1608–52
Open accessAbstract
Low-mass X-ray binaries (LMXBs) that show thermonuclear bursts are ideal sources for constraining the equation of state of neutron star matter. The lack of independent distance measurements for most of these sources, however, prevent a systematic exploration of the masses and radii of the neutron stars, hence limiting the equation-of-state studies. We present here a measurement of the distance to the LMXB 4U 1608−52 that is based on the study of the interstellar extinction toward the source. We first model the individual absorption edges of the elements Ne and Mg in the high-resolution X-ray spectrum obtained with XMM-Newton . We then combine this information with a measurement of the run of reddening with distance using red clump stars and determine a minimum distance to the source of 3.9 kpc, with a most probable value of 5.8 kpc. Finally, we analyze time-resolved X-ray spectra of Type I X-ray bursts observed from this source to measure the mass and the radius of the neutron star. We find a mass of M = 1.74 ± 0.14 M ☉ and a radius of R = 9.3 ± 1.0 km, respectively. This mass and radius can be achieved by several multi-nucleon equations of state.
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Thermonuclear (Type I) X‐Ray Bursts Observed by the Rossi X‐Ray Timing Explorer
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Self-citation
Cited by
Masses, Radii, and the Equation of State of Neutron Stars
Özel, F., & Freire, P. (2016) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081915-023322 · Cited by 1,354
Self-citationHinderer, T., Lackey, B. D., Lang, R. N., & Read, J. S. (2010) · Physical Review D · doi:10.1103/physrevd.81.123016 · Cited by 1,048
THE DENSE MATTER EQUATION OF STATE FROM NEUTRON STAR RADIUS AND MASS MEASUREMENTS
Özel, F., Psaltis, D., Güver, T., Baym, G., Heinke, C., & Guillot, S. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/820/1/28 · Cited by 403
Self-citationFurther stable neutron star models from f(R) gravity
Astashenok, A. V., Capozziello, S., & Odintsov, S. D. (2013) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2013/12/040 · Cited by 379
Maximal neutron star mass and the resolution of the hyperon puzzle in modified gravity
Astashenok, A. V., Capozziello, S., & Odintsov, S. D. (2014) · Physical Review D · doi:10.1103/physrevd.89.103509 · Cited by 255
Metadata
- Authors
- Güver, T., Özel, F., Cabrera-Lavers, A., & Wroblewski, P.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2010-03-09
- Volume
- 712
- Issue
- 2
- Pages
- 964-973
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W1992922395
- Cited by
- 321
- References
- 28
- FWCI
- 10.03
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Güver, T., Özel, F., Cabrera-Lavers, A., & Wroblewski, P. (2010). THE DISTANCE, MASS, AND RADIUS OF THE NEUTRON STAR IN 4U 1608–52. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/712/2/964
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