LEADER 02850oam 2200493 450 001 9910483648103321 005 20210415020851.0 010 $a3-662-62110-X 024 7 $a10.1007/978-3-662-62110-3 035 $a(CKB)4100000011515650 035 $a(DE-He213)978-3-662-62110-3 035 $a(MiAaPQ)EBC6381223 035 $a(PPN)255857128 035 $a(EXLCZ)994100000011515650 100 $a20210415d2021 uy 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 00$aTiming neutron stars $epulsations, oscillations and explosions /$fTomaso M. Belloni, Mariano Méndez, Chengmin Zhang, editors 205 $a1st ed. 2021. 210 1$aBerlin, Germany :$cSpringer,$d[2021] 210 4$d©2021 215 $a1 online resource (XII, 335 p. 92 illus., 58 illus. in color.) 225 1 $aAstrophysics and space science library ;$vVolume 461 300 $aIncludes index. 311 $a3-662-62108-8 327 $a1. Astrophysical Constraints on Dense Matter in Neutron Stars -- 2. General Relativity Measurements from Pulsars -- 3. Magnetars: A Short Review and Some Sparse Considerations -- 4. Accreting Millisecond X-ray Pulsars -- 5. Thermonuclear X-ray Bursts -- 6. High-Frequency Variability in Neutron-Star Low-Mass X-ray Binaries. 330 $aNeutron stars, whether isolated or in a binary system, display a varied and complex phenomenology, often accompanied by extreme variability of many time scales, which takes the form of pulsations due to the object rotation, quasi-periodicities associated to accretion of matter, and explosions due to matter accreted on the surface or to starquakes of highly magnetized objects. This book gives an overview of the current observational and theoretical standpoint in the research on the physics under the extreme conditions that neutron stars naturally provide. The six chapters explore three physical regions of a neutron star: the space around it, where accretion and pulsar companions allow testing of general relativity its surface, where millisecond pulsation and X-ray bursts provide clues about general relativistic effects and the equation of state of neutron matter its interior, of course, inaccessible to direct observations, can nevertheless, be probed with all observational parameters related to neutron star variability. 410 0$aAstrophysics and space science library ;$vVolume 461. 606 $aNeutron stars 615 0$aNeutron stars. 676 $a523.8874 702 $aBelloni$b Tomaso M. 702 $aMéndez$b Mariano 702 $aZhang$b Chengmin 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bUtOrBLW 906 $aBOOK 912 $a9910483648103321 996 $aTiming neutron stars$92830454 997 $aUNINA LEADER 01104nam 2200361 450 001 9910793795303321 005 20230802000649.0 010 $a3-8382-6079-1 035 $a(CKB)4100000008340173 035 $a(MiAaPQ)EBC5782397 035 $a(EXLCZ)994100000008340173 100 $a20190611d2012 uy 1 101 0 $ager 135 $aurcnu|||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aAnna, die alte Zauberin $e"der letzte Scheiterhaufen von Rotenburg" : Ein historischer Roman u?ber eine wahre Begebenheit /$fJu?rgen Hoops von Scheessel 210 1$aStuttgart :$cIbidem-Verlag,$d2012. 215 $a1 online resource (263 pages) $cillustrations 225 1 $aEdition Noe?ma 410 0$aEdition Noe?ma. 606 $aMagicians$vFiction 615 0$aMagicians 676 $a813.6 700 $aHoops von Scheessel$b Ju?rgen$01541707 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910793795303321 996 $aAnna, die alte Zauberin$93794054 997 $aUNINA