Impact of Low-Energy Cosmic Rays on Star Formation

被引:94
作者
Padovani, Marco [1 ]
Ivlev, Alexei V. [2 ]
Galli, Daniele [1 ]
Offner, Stella S. R. [3 ]
Indriolo, Nick [4 ]
Rodgers-Lee, Donna [5 ]
Marcowith, Alexandre [6 ]
Girichidis, Philipp [7 ]
Bykov, Andrei M. [8 ]
Kruijssen, J. M. [9 ]
机构
[1] INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy
[2] Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany
[3] Univ Texas Austin, Dept Astron, 2500 Speedway, Austin, TX 78712 USA
[4] Natl Inst Nat Sci, Natl Astron Observ Japan, ALMA Project, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
[5] Univ Dublin, Sch Phys, Trinity Coll Dublin, Coll Green, D02 PN40, Dublin 2, Dublin, Ireland
[6] Univ Montpellier, Lab Univers & Particules Montpellier, CNRS, UMR 5299, Pl E Bataillon,Cc072, F-34095 Montpellier, France
[7] Leibniz Inst Astrophys Potsdam AIP, Sternwarte 16, D-14482 Potsdam, Germany
[8] Ioffe Inst, Politehn Skaya 26, St Petersburg 194021, Russia
[9] Heidelberg Univ, Astron Rechen Inst, Zentrum Astron, Monchhofstr 12-14, D-69120 Heidelberg, Germany
基金
欧洲研究理事会;
关键词
Cosmic rays; Acceleration of particles; Astrochemistry; Magnetic fields; Protostars; Circumstellar discs; DIFFUSIVE SHOCK ACCELERATION; NARROW SELF-ABSORPTION; GALACTIC-CENTER; INTERSTELLAR-MEDIUM; MAGNETIC-FIELDS; MOLECULAR GAS; MODEL-CALCULATIONS; IONIZATION RATE; DARK CLOUDS; DENSE;
D O I
10.1007/s11214-020-00654-1
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In recent years, exciting developments have taken place in the identification of the role of cosmic rays in star-forming environments. Observations from radio to infrared wavelengths and theoretical modelling have shown that low-energy cosmic rays (<1 TeV) play a fundamental role in shaping the chemical richness of the interstellar medium, determining the dynamical evolution of molecular clouds. In this review we summarise in a coherent picture the main results obtained by observations and by theoretical models of propagation and generation of cosmic rays, from the smallest scales of protostars and circumstellar discs, to young stellar clusters, up to Galactic and extragalactic scales. We also discuss the new fields that will be explored in the near future thanks to new generation instruments, such as: CTA, for the gamma-ray emission from high-mass protostars; SKA and precursors, for the synchrotron emission at different scales; and ELT/HIRES, JWST, and ARIEL, for the impact of cosmic rays on exoplanetary atmospheres and habitability.
引用
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页数:57
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