1.0KMI - Nagoya Universityhttps://www.kmi.nagoya-u.ac.jp/engX-ray observations of the Galactic/Extragalactic Low-Mass X-ray Binaries - KMI - Nagoya Universityrich600338<blockquote class="wp-embedded-content" data-secret="fDSqHnH0mL"><a href="https://www.kmi.nagoya-u.ac.jp/eng/seminar/858/">X-ray observations of the Galactic/Extragalactic Low-Mass X-ray Binaries</a></blockquote><iframe sandbox="allow-scripts" security="restricted" src="https://www.kmi.nagoya-u.ac.jp/eng/seminar/858/embed/#?secret=fDSqHnH0mL" width="600" height="338" title="“X-ray observations of the Galactic/Extragalactic Low-Mass X-ray Binaries” — KMI - Nagoya University" data-secret="fDSqHnH0mL" frameborder="0" marginwidth="0" marginheight="0" scrolling="no" class="wp-embedded-content"></iframe><script type="text/javascript">
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Low-Mass X-ray Binaries (LMXBs) are luminous (typically, 10^32 – 10^39 erg s^-1 in the X-ray band) X-ray objects among the binary systems. The LMXB consists of a compact object such as neutron star (NS) or stellar-mass black hole (BH) and a low-mass companion. Matter from the companion star forms an “accretion disk” around the compact object, and then the accretion disk emits intense X-rays by the release of its gravitational potential energy. I will present the latest results of the X-ray observations of the Galactic and extragalactic LMXBs, …