Matches in SemOpenAlex for { <https://semopenalex.org/work/W1646125097> ?p ?o ?g. }
- W1646125097 endingPage "363" @default.
- W1646125097 startingPage "345" @default.
- W1646125097 abstract "X-ray emission is a common feature of all varieties of isolated neutron stars (INS) and, thanks to the advent of sensitive instruments with good spectroscopic, timing, and imaging capabilities, X-ray observations have become an essential tool in the study of these objects. Non-thermal X-rays from young, energetic radio pulsars have been detected since the beginning of X-ray astronomy, and the long-sought thermal emission from cooling neutron star's surfaces can now be studied in detail in many pulsars spanning different ages, magnetic fields, and, possibly, surface compositions. In addition, other different manifestations of INS have been discovered with X-ray observations. These new classes of high-energy sources, comprising the nearby X-ray Dim Isolated Neutron Stars, the Central Compact Objects in supernova remnants, the Anomalous X-ray Pulsars, and the Soft Gamma-ray Repeaters, now add up to several tens of confirmed members, plus many candidates, and allow us to study a variety of phenomena unobservable in standard'' radio pulsars." @default.
- W1646125097 created "2016-06-24" @default.
- W1646125097 creator A5014665960 @default.
- W1646125097 date "2010-12-14" @default.
- W1646125097 modified "2023-10-12" @default.
- W1646125097 title "X-ray emission from isolated neutron stars" @default.
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