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곽규진

Kwak, Kyujin
Computational Astrophysics Lab.
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dc.citation.conferencePlace KO -
dc.citation.title 14th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG2017 -
dc.citation.volume 1947 -
dc.contributor.author Kwak, Kyujin -
dc.contributor.author Lee, Chang-Hwan -
dc.contributor.author Kim, Myungkuk -
dc.contributor.author Kim, Young-Min -
dc.date.accessioned 2023-12-19T18:39:20Z -
dc.date.available 2023-12-19T18:39:20Z -
dc.date.created 2018-11-01 -
dc.date.issued 2017-06-27 -
dc.description.abstract The mass and radius of neutron star (NS) in the low mass X-ray binary (LMXB) can be measured simultaneously from the evolving spectra of the photospheric radius expansion (PRE) X-ray bursts (XRBs). Precise measurements require the distance to the target, information on the radiating surface, and the composition of accreted material. Future observations with large ground-based telescopes such as Giant Magellan Telescope (GMT) and Thirty Meter Telescope (TMT) may reduce the uncertainties in the estimation of the mass and radius of NS because they could provide information on the composition of accreted material by identifying the companion stars in LMXBs. We investigate these possibilities and present our results for selected targets. -
dc.identifier.bibliographicCitation 14th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG2017, v.1947 -
dc.identifier.doi 10.1063/1.5030812 -
dc.identifier.isbn 978-073541642-0 -
dc.identifier.issn 0094-243X -
dc.identifier.scopusid 2-s2.0-85047469132 -
dc.identifier.uri https://scholarworks.unist.ac.kr/handle/201301/37527 -
dc.identifier.url https://aip.scitation.org/doi/abs/10.1063/1.5030812 -
dc.language 영어 -
dc.publisher 14th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG2017 -
dc.title Constraining the mass and radius of neutron star by future observations -
dc.type Conference Paper -
dc.date.conferenceDate 2017-06-27 -

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