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- W2976207965 endingPage "106901" @default.
- W2976207965 startingPage "106901" @default.
- W2976207965 abstract "Young and rotation-powered neutron stars (NSs) are commonly observed as rapidly-spinning pulsars. They dissipate their rotational energy by emitting pulsar wind with electromagnetic radiation and spin down at a steady rate, according to the simple steadily-rotating magnetic dipole model. In reality, however, multiwavelength observations of radiation from the NS surface and magnetosphere have revealed that the evolution and properties of NSs are highly diverse, often dubbed as 'NS zoo'. In particular, many of young and highly magnetized NSs show a high degree of activities, such as sporadic electromagnetic outbursts and irregular changes in pulse arrival times. Importantly, their magnetic field, which are the strongest in the universe, makes them ideal laboratories for fundamental physics. A class of highly-magnetized isolated NSs is empirically divided into several subclasses. In a broad classification, they are, in the order of the magnetic field strength (B) from the highest, 'magnetars' (historically recognized as soft gamma-ray repeaters and/or anomalous x-ray pulsars), 'high-B pulsars', and (nearby) x-ray isolated NSs. This article presents an introductory review for non-astrophysicists about the observational properties of highly-magnetized NSs, and their implications. The observed dynamic nature of NSs must be interpreted in conjunction with transient magnetic activities triggered during magnetic-energy dissipation process. In particular, we focus on how the five fundamental quantities of NSs, i.e. mass, radius, spin period, surface temperature, and magnetic fields, as observed with modern instruments, change with evolution of, and vary depending on the class of, the NSs. They are the foundation for a future unified theory of NSs." @default.
- W2976207965 created "2019-10-03" @default.
- W2976207965 creator A5006508369 @default.
- W2976207965 creator A5060270008 @default.
- W2976207965 creator A5060752473 @default.
- W2976207965 date "2019-09-24" @default.
- W2976207965 modified "2023-10-14" @default.
- W2976207965 title "Observational diversity of magnetized neutron stars" @default.
- W2976207965 cites W1481638055 @default.
- W2976207965 cites W1497620729 @default.
- W2976207965 cites W1509022852 @default.
- W2976207965 cites W1515675433 @default.
- W2976207965 cites W1519557512 @default.
- W2976207965 cites W1530212668 @default.
- W2976207965 cites W1534966610 @default.
- W2976207965 cites W1540565992 @default.
- W2976207965 cites W1555220461 @default.
- W2976207965 cites W1561146689 @default.
- W2976207965 cites W1573526496 @default.
- W2976207965 cites W1583674215 @default.
- W2976207965 cites W1601277342 @default.
- W2976207965 cites W1621979734 @default.
- W2976207965 cites W1646125097 @default.
- W2976207965 cites W1652036496 @default.
- W2976207965 cites W1653349128 @default.
- W2976207965 cites W165507508 @default.
- W2976207965 cites W1657638373 @default.
- W2976207965 cites W1664336417 @default.
- W2976207965 cites W1675800434 @default.
- W2976207965 cites W1742245113 @default.
- W2976207965 cites W1766331502 @default.
- W2976207965 cites W1829911009 @default.
- W2976207965 cites W1855373758 @default.
- W2976207965 cites W1862196932 @default.
- W2976207965 cites W1862641251 @default.
- W2976207965 cites W1868967526 @default.
- W2976207965 cites W1882454150 @default.
- W2976207965 cites W1922264974 @default.
- W2976207965 cites W1929472048 @default.
- W2976207965 cites W1930867846 @default.
- W2976207965 cites W1938091735 @default.
- W2976207965 cites W1950634084 @default.
- W2976207965 cites W1955505268 @default.
- W2976207965 cites W1964569342 @default.
- W2976207965 cites W1967542460 @default.
- W2976207965 cites W1967583406 @default.
- W2976207965 cites W1967825921 @default.
- W2976207965 cites W1967953542 @default.
- W2976207965 cites W1968160375 @default.
- W2976207965 cites W1968199171 @default.
- W2976207965 cites W1969416246 @default.
- W2976207965 cites W1970455611 @default.
- W2976207965 cites W1970722374 @default.
- W2976207965 cites W1970818525 @default.
- W2976207965 cites W1972524869 @default.
- W2976207965 cites W1973069147 @default.
- W2976207965 cites W1973311828 @default.
- W2976207965 cites W1973548823 @default.
- W2976207965 cites W1973820399 @default.
- W2976207965 cites W1974420904 @default.
- W2976207965 cites W1975478554 @default.
- W2976207965 cites W1975689236 @default.
- W2976207965 cites W1975878427 @default.
- W2976207965 cites W1977051691 @default.
- W2976207965 cites W1977299014 @default.
- W2976207965 cites W1977803258 @default.
- W2976207965 cites W1977998389 @default.
- W2976207965 cites W1978505636 @default.
- W2976207965 cites W1978910296 @default.
- W2976207965 cites W1978911181 @default.
- W2976207965 cites W1978970854 @default.
- W2976207965 cites W1979368580 @default.
- W2976207965 cites W1980224506 @default.
- W2976207965 cites W1981256261 @default.
- W2976207965 cites W1981266089 @default.
- W2976207965 cites W1981557052 @default.
- W2976207965 cites W1981678068 @default.
- W2976207965 cites W1982552086 @default.
- W2976207965 cites W1982997995 @default.
- W2976207965 cites W1983233507 @default.
- W2976207965 cites W1983880878 @default.
- W2976207965 cites W1984409509 @default.
- W2976207965 cites W1984829288 @default.
- W2976207965 cites W1986515303 @default.
- W2976207965 cites W1986547154 @default.
- W2976207965 cites W1986864016 @default.
- W2976207965 cites W1987418066 @default.
- W2976207965 cites W1987796387 @default.
- W2976207965 cites W1988596177 @default.
- W2976207965 cites W1989980321 @default.
- W2976207965 cites W1990494221 @default.
- W2976207965 cites W1991234572 @default.
- W2976207965 cites W1992106524 @default.
- W2976207965 cites W1992420274 @default.
- W2976207965 cites W1992768712 @default.
- W2976207965 cites W1993307992 @default.
- W2976207965 cites W1993495528 @default.
- W2976207965 cites W1994303408 @default.