TY - GEN A1 - Paerels, Frits A1 - Kaastra, Jelle A1 - Ohashi, Takaya A1 - Richter, Philipp A1 - Bykov, Andrei A1 - Nevalainen, Jukka T1 - Future instrumentation for the study of the warm-hot intergalactic medium T2 - Postprints der Universität Potsdam : Mathematisch Naturwissenschaftliche Reihe N2 - We briefly review capabilities and requirements for future instrumentation in UV- and X-ray astronomy that can contribute to advancing our understanding of the diffuse, highly ionised intergalactic medium. T3 - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe - 859 KW - instrumentation: spectrographs KW - instrumentation: photometers KW - ultraviolet: general KW - x-rays: general KW - γ -rays: general Y1 - 2020 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-434057 SN - 1866-8372 IS - 859 SP - 405 EP - 418 ER - TY - JOUR A1 - Bykov, Andrei A1 - Gehrels, Neil A1 - Krawczynski, Henric A1 - Lemoine, Martin A1 - Pelletier, Guy A1 - Pohl, Martin T1 - Particle acceleration in relativistic outflows JF - Space science reviews N2 - In this review we confront the current theoretical understanding of particle acceleration at relativistic outflows with recent observational results on various source classes thought to involve such outflows, e.g. gamma-ray bursts, active galactic nuclei, and pulsar wind nebulae. We highlight the possible contributions of these sources to ultra-high-energy cosmic rays. KW - Cosmic rays KW - Particle acceleration KW - Shocks Y1 - 2012 U6 - https://doi.org/10.1007/s11214-012-9896-y SN - 0038-6308 VL - 173 IS - 1-4 SP - 309 EP - 339 PB - Springer CY - Dordrecht ER - TY - JOUR A1 - Herbst, Konstantin A1 - Baalmann, Lennart R. A1 - Bykov, Andrei A1 - Engelbrecht, N. Eugene A1 - Ferreira, Stefan E. S. A1 - Izmodenov, Vladislav V. A1 - Korolkov, Sergey D. A1 - Levenfish, Ksenia P. A1 - Linsky, Jeffrey L. A1 - Meyer, Dominique M. -A. A1 - Scherer, Klaus A1 - Strauss, R. Du Toit T1 - Astrospheres of planet-hosting cool stars and beyond when modeling meets observations JF - Space science reviews N2 - Thanks to dedicated long-term missions like Voyager and GOES over the past 50 years, much insight has been gained on the activity of our Sun, the solar wind, its interaction with the interstellar medium, and, thus, about the formation, the evolution, and the structure of the heliosphere. Additionally, with the help of multi-wavelength observations by the Hubble Space Telescope, Kepler, and TESS, we not only were able to detect a variety of extrasolar planets and exomoons but also to study the characteristics of their host stars, and thus became aware that other stars drive bow shocks and astrospheres. Although features like, e.g., stellar winds, could not be measured directly, over the past years several techniques have been developed allowing us to indirectly derive properties like stellar mass-loss rates and stellar wind speeds, information that can be used as direct input to existing astrospheric modeling codes. In this review, the astrospheric modeling efforts of various stars will be presented. Starting with the heliosphere as a benchmark of astrospheric studies, investigating the paleo-heliospheric changes and the Balmer H alpha projections to 1 pc, we investigate the surroundings of cool and hot stars, but also of more exotic objects like neutron stars. While pulsar wind nebulae (PWNs) might be a source of high-energy galactic cosmic rays (GCRs), the astrospheric environments of cool and hot stars form a natural shield against GCRs. Their modulation within these astrospheres, and the possible impact of turbulence, are also addressed. This review shows that all of the presented modeling efforts are in excellent agreement with currently available observations. KW - Magneto-hydrodynamic modeling KW - Stochastic differential equations KW - Galactic cosmic rays KW - Heliosphere KW - Astrosphere Y1 - 2022 U6 - https://doi.org/10.1007/s11214-022-00894-3 SN - 0038-6308 SN - 1572-9672 VL - 218 IS - 4 PB - Springer Nature CY - Dordrecht ER -