Test of Galactic Cosmic-Ray source models

Space Science Reviews

Volumn 99, Issue 1-4, 2001, Pages 329-352

  Drury, L O'C ^a   Ellison, D E ^b   Aharonian, F A ^c   Berezhko, E ^d   Bykov, A ^e   Decourchelle, A ^f   Diehl, R ^g   Meynet, G ^h   Parizot, E ^a,i   Raymond, J ^j   Reynolds, S ^b   Spangler, S ^k  

^a DUBLIN INSTITUTE FOR ADVANCED STUDIES   (Ireland)

^b NORTH CAROLINA STATE UNIVERSITY   (United States)

^c MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^d YU G SHAFER INSTITUTE OF COSMOPHYSICAL RESEARCH AND AERONOMY   (Russian Federation)

^e IOFFE INSTITUTE   (Russian Federation)

^f UNIVERSITÉ PARIS DIDEROT   (France)

^g MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^h UNIVERSITÉ DE GENÈVE   (Switzerland)

ⁱ 91405 Orsay Campus   (France)

^j HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^k UNIVERSITY OF IOWA   (United States)

more..

Author keywords

[No Author keywords available]

Indexed keywords

ACCELERATION; ASTRONOMY; CONFERENCE PAPER; COSMIC RADIATION; ELECTRON; GAMMA RADIATION; MODEL; PHYSICS; SYNCHROTRON; X RAY ANALYSIS;

EID: 20244373712     PISSN: 00386308     EISSN: None     Source Type: Journal    
DOI: 10.1023/A:1013825905795     Document Type: Conference Paper

References (102)

1. Evidence for enhanced MHD turbulence outside sharp-rimmed supernova remnants
2. Evidence of X-ray synchrotron emission from electrons accelerated to 40 TeV in the supernova remnant cassiopeia A
3. Stellar nucleosynthesis and the cosmic-ray source composition up to Zn
4. ROSAT All-sky survey map of the cygnus loop: Overall structure and comparison with radio map
5. The hard X-ray emission of the young supernova remnants
6. Radio to gamma-ray emission from shell-type supernova remnants: Predictions from nonlinear shock acceleration models
7. Maximum energy of cosmic rays accelerated by supernova shocks
8. A simple model of nonlinear diffusive shock acceleration
9. TeV gamma rays expected from supernova remnants in different uniform interstellar media
10. Particle acceleration at astrophysical shocks - A theory of cosmic-ray origin
11. Giant molecular clouds
12. The warm insterstellar medium around the cygnus loop
13. Application of cosmic-ray shock theories to the cygnus loop - An alternative model
14. Thermal and nonthermal X-ray emission in SNR RCW 86
15. Constraints on cosmic-ray origin from TeV gamma-ray observations of supernova remnants
16. Nonthermal particles in star forming regions
17. Effect of shocks on interstellar turbulence and cosmic-ray dynamics
18. On non-thermal particle generation in superbubbles
19. Primary cosmic ray composition around the knee in the model of particle acceleration by shock front ensemble in galactic superbubbles
20. Electron kinetics in collisionless shock waves
21. Optical emission from a fast shock wave: The remnants of Tycho's supernova and SN 1006
22. Blast waves with cosmic-ray pressure
23. The optical emission from a fast shock wave with application to supernova remnants
24. High resolution measurements of the isotopic composition of Galactic Cosmic Ray C, N, 0, Mg and Si from the Ulysses HET
25. Light element abundance patterns in the orion association: I) HST observations of boron in G-dwarfs
26. Thermal X-ray emission and cosmic-ray production in young supernova remnants
27. Quantitative analysis of WC stars: Constraints on neon abundances from ISO-SWS spectroscopy
28. Time dependent acceleration of test-particles at shocks
29. The gamma-ray visibility of supernova remnants. A test of cosmic ray origin
30. The isotopic composition of Galactic Cosmic-Ray elements from carbon to silicon: The combined release and radiation effects satellite investigation
31. Spatially resolved analysis of X-ray synchrotron emission in supernova remnants
32. The cosmic ray - X-ray connection: Effects of nonlinear shock acceleration on photon production in SNRs
33. A determination of relativistic shock jump conditions using Monte Carlo techniques
34. Galactic Cosmic Rays from supernova remnants. II. Shock acceleration of gas and dust
35. Nonlinear shock acceleration and photon emission in supernova remnants
36. The origin of PeV cosmic rays
37. A two-dimensional spectrum of a nonradiative shock filament in the cygnus loop
38. The asymmetric radio remnant of SN 1987A
39. Chandra X-ray observatory arcsecond imaging of the young, oxygen-rich supernova remnant IE 0102.2-7219
40. Cosmic ray source abundances and the acceleration of cosmic rays
41. The balmer-dominated NE limb of the cygnus loop supernova remnant
42. Cosmic ray acceleration from supernova ejecta in superbubbles
43. The extraordinarily rapid expansion of the X-ray remnant of Kepler's supernova (SN 1604)
44. The expansion of the X-ray remnant of Tycho's supernova (SN 1572)
45. Electron heating and cosmic rays at a supernova shock from chandra X-ray observations of IE 0102.2-7219
46. Shock acceleration of cosmic rays - A critical review
47. Newly synthesized lithium in the interstellar medium
48. The X-ray expansion of the supernova remnant cassiopeia A
49. Evolution superbubble in a turbulent, multi-phased and magnetized ISM
50. Evidence for shock acceleration of high-energy electrons in the supernova remnant SN:1006
51. Discovery of Non-Thermal X-Rays from the Northwest Shell of the New SNR RX J1713.7-3946: The second SN 1006?
52. Non-radiative shocks associated with SN 1006
53. Accelerated electrons in cassiopeia A: An explanation for the hard X-ray tail
54. Supernovae, supernova remnants and stellar winds
55. Non-linear amplification of a magnetic field driven by cosmic ray streaming
56. Cosmic-ray isotopic composition of C, N, O, Ne, Mg, Si nuclei in the energy range 50-2000 MeV per nucleon measured by the voyager spacecraft during the solar minimum period
57. Superbubbles in disk galaxies
58. Isotopic anomalies in cosmic rays and winds from Wolf-Rayet stars: A new model
59. The production of the elements Li, Be, B by Galactic Cosmic Rays in space and its relation with stellar observations
60. Galactic Cosmic Rays from supernova remnants. I. A cosmic-ray composition controlled by volatility and mass-to-charge ratio
61. Wolf-Rayet stars and isotopic anomalies in cosmic rays
62. Radio observations of SN 1980K: Evidence for rapid presupernova evolution
63. Radio observations of SN 1979C: Evidence for rapid presupernova evolution
64. Hubble space telescope observations of oxygen-rich supernova remnants in the Magellanic cloud. I. Narrow-band imaging of N132D in the LMC
65. High energy gamma-ray emission from supernova remnants
66. The effect of a non-maxwellian electron distribution on oxygen and iron ionization balances in the solar corona
67. The orion gamma-ray emission and the orion-eridanus bubble
68. 6Li, Be and B
69. Spallative nucleosynthesis in supernova remnants. I. Analytical estimates
70. Spallative nucleosynthesis in supernova remnants. II. Time dependent numerical results
71. The supernova remnant CTA1 (G 119.5+10.3): A study of the breakout phenomenon
72. The effects of a hybrid maxwellian/power-law electron distribution on the ionisation balance
73. Neutron capture nucleosynthesis during core helium burning in massive stars
74. The X-ray spectrum of the supernova remnant 1E 0102.2-7219
75. Detection of ultraviolet emission lines in SN 1006 with the Hopkins ultraviolet telescope
76. SOHO and radio observations of a CME shock wave
77. Galactic Cosmic Ray origin of Li, Be and B in stars
78. Synchrotron models for X-rays from the supernova remnant SN 1006
79. Models of synchrotron X-rays from shell supernova remnants
80. Electron acceleration in Tycho's and Kepler's supernova remnants - Spectral evidence of fermi shock acceleration
81. Maximum energies of shock-accelerated electrons in young shell supernova remnants
82. The environs of Tycho's supernova remnant explored through the HI 21 centimeter line
83. Electron heating and the potential jump across fast mode shocks
84. Nonthermal X-Ray Emission from the Shell-Type Supernova Remnant G347.3-0.5
85. RXJ0852.0-0462: Another nonthermal shell-type SNR (G266.2-1.2)
86. High-resolution spectroscopy of balmer-dominated shocks in the large Magellanic cloud
87. [NEv] imaging of the cygnus loop
88. Discovery of TeV gamma rays from SN 1006: Further evidence for the supernova remnant origin of cosmic rays
89. CGRO/OSSE observations of the cassiopeia A SNR
90. Superbubbles in magnetized interstellar media
91. Evolution of nonradiative supernova remnants
92. The expansion of cassiopeia A as seen in X-rays
93. Diffusive shock acceleration of energetic electrons subject to synchrotron losses
94. Radio emission from supernovae. II. - SN 1986J: A different kind of type II
95. Cosmic-ray isotopic composition results from the ACE mission
96. ISO SWS spectroscopy of WR 146 (WC6+O)
97. Properties of Wolf-Rayet stars from X-ray to radio data
98. Anomalous isotopic composition of cosmic rays