CLUSTERS OF GALAXIES: SHOCK WAVES AND COSMIC RAYS |
RYU DONGSU
(Department of Astronomy & Space Science, Chungnam National University)
KANG HYESUNG (Department of Earth Sciences, Pusan National University) |
1 |
Hot Gas in the CDM Scenario: X-Ray Clusters from a High Resolution Numerical Simulation
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DOI |
2 |
where Are the Baryons?
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DOI ScienceOn |
3 |
Cosmic Ray Protons Accelerated at Cosmological Shocks and Their Impact on Groups and Clusters of Galaxies
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DOI ScienceOn |
4 |
EGRET Observations of the North Galactic Pole Region
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DOI ScienceOn |
5 |
A Cosmological Hydrodynamic Code Based on the Total Variation Diminishing Scheme
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DOI |
6 |
Accreting Matter around Clusters of Galaxies: One-Dimensional Considerations
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DOI ScienceOn |
7 |
The Protogalactic Origin for Cosmic Magnetic Fields
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DOI ScienceOn |
8 |
Cluster Accretion Shocks as Possible Acceleration Sites for Ultra High Energy Protons below the Greisen Cutoff
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DOI ScienceOn |
9 |
A New Radio-X-Ray Probe of Galaxy Cluster Magnetic Fields
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DOI ScienceOn |
10 |
Particle Acceleration at Astrophysical Shocks-a Theory of Cosmic-Ray Origin
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DOI ScienceOn |
11 |
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12 |
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13 |
Properties of Cosmic Shock Waves in Large Scale Structure Formation
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DOI ScienceOn |
14 |
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15 |
Cosmic Shock Waves on Large Scales of the Universe
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16 |
Discovery of Intergalactic Radio Emission in the Coma-A1367 Supercluster
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DOI |
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