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곽규진

Kwak, Kyujin
Computational Astrophysics Lab.
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Estimating Mass and Radius of a Neutron Star in Low-Mass X-ray Binary

Author(s)
Kwak, KyujinSung, Kwang HyunKim, Young-MinKim, MyungkukLee, Chang-Hwan
Issued Date
2019-04-11
URI
https://scholarworks.unist.ac.kr/handle/201301/80016
Fulltext
http://www.kas.org/html/sub4_01_view.html?gubun=1&idx=61
Citation
2019년 봄 제100차 한국천문학회 학술대회
Abstract
Mass and radius of a neutron star in low-mass X-ray binary (LMXB) can be estimated simultaneously when the observed light curve and spectrum show the photospheric radius expansion feature. This method has been applied to 4U 1746-37 and the mass and radius were found to be unusually small in comparison with typical neutron stars. We re-estimate the mass and radius of this target by considering that the observed light curve and spectrum can be affected by other X-ray sources because this LMXB belongs to a very crowded globular cluster NGC 6441. The new estimation increases the mass and radius but they do not reach the typical values yet.
Publisher
한국천문학회
ISSN
1226-2692

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