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Titlebook: Galactic High-Energy Astrophysics High-Accuracy Timing and Positional Astronomy; Lectures Held at the J. Paradijs,H. M. Maitzen Conference

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11#
發(fā)表于 2025-3-23 11:47:39 | 只看該作者
https://doi.org/10.1007/3-540-56874-3Accretion; Astrometrie; Astrometry; Astronomie; Astronomy; Astrophysik; Raumforschung; Space Research; astro
12#
發(fā)表于 2025-3-23 15:14:45 | 只看該作者
Conference proceedings 1993ccelerations(including shocks), the interstellar medium andsupernovaeremnants, high-energy emissions from normal starsandaccretion in close binaries. The second part deals withobservationslike pulsar timing, and its measurement withradioastronomical tools, and astrometry, as performed in theHIPPARCOS satellite program.
13#
發(fā)表于 2025-3-23 19:14:20 | 只看該作者
14#
發(fā)表于 2025-3-24 00:48:32 | 只看該作者
Olexandr I. Skibinskyi,Andriy O. Hnatiukgnetic field axes. The star‘s rotation sweeps one of the beams past the Earth to create the observed pulse if the axis is tilted with respect to the rotation axis. New classes of pulsars - including ones with millisecond rotation periods - have been discovered in the last decade. The rotations of pu
15#
發(fā)表于 2025-3-24 04:05:46 | 只看該作者
16#
發(fā)表于 2025-3-24 07:11:31 | 只看該作者
17#
發(fā)表于 2025-3-24 14:14:53 | 只看該作者
18#
發(fā)表于 2025-3-24 17:29:08 | 只看該作者
Joanna M. Jenkinson,Nicholas J. TalbotThe current status of theories of the interstellar medium as well as of supernova remnants is reviewed. Some shortcomings and the importance of including magnetic fields and cosmic rays are discussed in detail and at the end this additional physical input is compared to observations in the X- and γ-range.
19#
發(fā)表于 2025-3-24 19:31:26 | 只看該作者
Particle acceleration in astrophysics,I review the physical principles of particle acceleration in astrophysical objects, with an emphasis on diffusive shock acceleration.
20#
發(fā)表于 2025-3-25 00:01:14 | 只看該作者
Interstellar medium and supernova remnants,The current status of theories of the interstellar medium as well as of supernova remnants is reviewed. Some shortcomings and the importance of including magnetic fields and cosmic rays are discussed in detail and at the end this additional physical input is compared to observations in the X- and γ-range.
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