Astrophysics Update 2
https://doi.org/10.1007/3-540-30313-8
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https://doi.org/10.1007/3-540-30313-8
https://doi.org/10.1016/c2009-0-10963-7
Radio astronomy and high-energy astrophysics The early history of radio astronomy was recounted in Section 7.3; that story ended in the mid 1950s, by which time the Galactic and extragalactic nature of the discrete radio sources was establi...
https://doi.org/10.1017/cbo9781139878319.012
What role does viscosity play in accretion discs? How do you calculate the 'glitch function' of a pulsar? And can strong shocks account for the energy spectrum of electrons in our Galaxy? These are just some of the exciting questions that P...
https://doi.org/10.1017/cbo9781139170505
https://doi.org/10.1007/978-1-4613-1897-2
C A Barnes, D D Clayton and D N Schramm (eds) 1982 Cambridge: Cambridge University Press xiii + 562 pp price £40 This collection of 23 articles reviews all the many aspects of nuclear astrophysics, from solar system abundances to particle p...
https://doi.org/10.1088/0031-9112/34/5/028
Designed for teaching astrophysics to physics students at advanced undergraduate or beginning graduate level, this textbook also provides an overview of astrophysics for astrophysics graduate students, before they delve into more specialize...
https://doi.org/10.1017/cbo9780511802218
106 On the birth and development of cosmic-ray astrophysics novae and other stars, the role of acceleration near the galactic center). Also related is the problem of cosmic-ray acceleration and propagation in radio galaxies and quasars....
https://doi.org/10.1201/9780367801618-22
We model the formation of star clusters in a dwarf galaxy progenitor during the first 700 Myr of cosmic history using a cosmological radiation-hydrodynamic simulation with a sub-grid star formation efficiency (SFE) model calibrated from AU-...
10.33232/001c.145064
Long period radio transients (LPTs) are the slowest radio-pulsing sources ever found, with the current population spanning periods of seven minutes to over six hours. Two of the thirteen published LPTs, ILT J1101+5521 and GLEAM-X J0704--37,...
10.33232/001c.167716
The TeV diffuse emission from the Galactic plane is produced by multi TeV electrons and nuclei interacting with radiation fields and ambient gas, respectively. Measurements of the TeV diffuse emission help constrain CR origin and transport ...
10.3389/fspas.2018.00008
Accretion Power in Astrophysics examines accretion as a source of energy in both binary star systems containing compact objects, and in active galactic nuclei. Assuming a basic knowledge of physics, the authors describe the physical process...
https://doi.org/10.1017/cbo9781139164245
Providing students with an in-depth account of the astrophysics of high energy phenomena in the Universe, the third edition of this well-established textbook is ideal for advanced undergraduate and beginning graduate courses in high energy ...
https://doi.org/10.1017/cbo9780511778346
https://doi.org/10.1051/epn/19750612003
The Astrophysics Source Code Library (ASCL), founded in 1999, is a free on-line registry for source codes of interest to astronomers and astrophysicists. The library is housed on the discussion forum for Astronomy Picture of the Day (APOD) ...
https://doi.org/10.48550/arxiv.1212.1916
https://doi.org/10.1016/0031-9201(70)90034-8
Editor's preface. I. The astrophysics of cosmic rays (general review). II. General information on cosmic rays and on the interstellar medium. III. The proton-nuclear component of cosmic rays in the Galaxy. General questions. Chemical and is...
https://doi.org/10.9783/9781512803761-008