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- W1562289969 abstract "Relativistic strongly magnetized winds outflowing from fast-rotating compact objects like millisecond pulsars with surface magnetic fields of $sim 10^{15}-10^{16}$ G are plausible sources of cosmological $gamma$-ray bursts. In such winds, there are at least three regions where extremely powerful X-ray and $gamma$-ray emission may be generated. The first radiating region is the wind photosphere that is at a distance of $sim 10^9$ cm from the compact object. The second radiating region is at a distance of $sim 10^{13}-10^{14}$ cm. In this region, the striped component of the wind field is transformed into large-amplitude electromagnetic waves. The third radiating region is at a distance of $sim 10^{16}-10^{17}$ cm, where deceleration of the wind due to its interaction with an ambient medium becomes important. Radiation from all these regions is considered." @default.
- W1562289969 created "2016-06-24" @default.
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- W1562289969 date "1999-09-26" @default.
- W1562289969 modified "2023-09-27" @default.
- W1562289969 title "Radiation from Relativistic Strongly Magnetized Outflows" @default.
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