001432346 000__ 03811cam\a2200589\i\4500 001432346 001__ 1432346 001432346 003__ OCoLC 001432346 005__ 20230309003437.0 001432346 006__ m\\\\\o\\d\\\\\\\\ 001432346 007__ cr\un\nnnunnun 001432346 008__ 201107t20212021gw\a\\\\ob\\\\001\0\eng\d 001432346 019__ $$a1202061262$$a1224379699$$a1225367413$$a1228842689$$a1229919028 001432346 020__ $$a366262110X$$qelectronic book 001432346 020__ $$a9783662621103$$q(electronic bk.) 001432346 020__ $$z9783662621080$$qhardback 001432346 020__ $$z3662621088$$qhardback 001432346 0247_ $$a10.1007/978-3-662-62110-3$$2doi 001432346 035__ $$aSP(OCoLC)1204136715 001432346 040__ $$aEBLCP$$beng$$epn$$erda$$cEBLCP$$dOCLCO$$dYDX$$dGZM$$dGW5XE$$dSFB$$dUKAHL$$dOCLCO$$dOCLCF$$dUPM$$dOCL$$dOCLCQ$$dOCLCO$$dCOM$$dWAU$$dN$T$$dOCLCQ 001432346 049__ $$aISEA 001432346 050_4 $$aQB843.N4 001432346 08204 $$a523.8/874$$223 001432346 24500 $$aTiming neutron stars :$$bpulsations, oscillations and explosions /$$cTomaso M. Belloni, Mariano Méndez, Chengmin Zhang, editors. 001432346 264_1 $$aBerlin, Germany :$$bSpringer,$$c[2021] 001432346 264_4 $$c©2021 001432346 300__ $$a1 online resource (xii, 335 pages) :$$bIllustrations. 001432346 336__ $$atext$$btxt$$2rdacontent 001432346 336__ $$astill image$$bsti$$2rdacontent 001432346 337__ $$acomputer$$bc$$2rdamedia 001432346 338__ $$aonline resource$$bcr$$2rdacarrier 001432346 347__ $$atext file 001432346 347__ $$bPDF 001432346 4901_ $$aAstrophysics and space science library,$$x2214-7985 ;$$vvolume 461 001432346 504__ $$aIncludes bibliographical references and index. 001432346 5050_ $$a1. Astrophysical constraints on dense matter in neutron stars / M. Coleman Miller -- 2. General relativity measurements from pulsars / Marta Burgay, Delphine Perrodin, Andrea Possenti -- 3. Magnetars : A short review and some sparse considerations / Paolo Esposito, Nanda Rea, Gian Luca Israel -- 4. Accreting millisecond X-ray pulsars / Alessandro Patruno, Anna L. Watts -- 5. Thermonuclear X-ray bursts / Duncan K. Galloway, Laurens Keek -- 6. High-frequency variability in neutron-star low-mass X-ray binaries / Mariano Méndez, Tomaso M. Belloni. 001432346 506__ $$aAccess limited to authorized users. 001432346 520__ $$aNeutron stars, whether isolated or in a binary system, display a varied and complex phenomenology, often accompanied by extreme variability of many time scales, which takes the form of pulsations due to the object rotation, quasi-periodicities associated to accretion of matter, and explosions due to matter accreted on the surface or to starquakes of highly magnetized objects. This book gives an overview of the current observational and theoretical standpoint in the research on the physics under the extreme conditions that neutron stars naturally provide. The six chapters explore three physical regions of a neutron star: the space around it, where accretion and pulsar companions allow testing of general relativity its surface, where millisecond pulsation and X-ray bursts provide clues about general relativistic effects and the equation of state of neutron matter its interior, of course, inaccessible to direct observations, can nevertheless, be probed with all observational parameters related to neutron star variability. 001432346 588__ $$aDescription based on print version record. 001432346 650_0 $$aNeutron stars. 001432346 650_6 $$aÉtoiles à neutrons. 001432346 655_0 $$aElectronic books. 001432346 7001_ $$aBelloni, T.$$q(Tomaso),$$eeditor. 001432346 7001_ $$aMéndez, Mariano,$$eeditor. 001432346 7001_ $$aZhang, Chengmin,$$eeditor. 001432346 77608 $$iPrint version:$$tTiming neutron stars.$$dBerlin : Springer, [2021]$$z9783662621080$$w(OCoLC)1223316456 001432346 830_0 $$aAstrophysics and space science library ;$$vv. 461. 001432346 852__ $$bebk 001432346 85640 $$3Springer Nature$$uhttps://univsouthin.idm.oclc.org/login?url=https://link.springer.com/10.1007/978-3-662-62110-3$$zOnline Access$$91397441.1 001432346 909CO $$ooai:library.usi.edu:1432346$$pGLOBAL_SET 001432346 980__ $$aBIB 001432346 980__ $$aEBOOK 001432346 982__ $$aEbook 001432346 983__ $$aOnline 001432346 994__ $$a92$$bISE