Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
JILA, University of Colorado
JILA, U. of Colorado
JILA, Univ. of Colorado
JILA, University of Colorado at Boulder
JILA, Boulder, CO
JILA, Boulder, USA
JILA - University of Colorado
Jila
JILA, University of Colorado, Boulder, USA
University of Colorado
Joint Institute for Laboratory Astrophysics, Boulder, CO
Joint Institute for Laboratory Astrophysics, University of Colorado and National Institute of Standards and Technology, Campus Box 440, Boulder, CO 80309-0440, USA
Joint Institute for Laboratory Astrophysics; Colorado, University, Boulder
Joint Inst. for Lab. Astrophysics
Colorado Univ., Boulder, CO.
University of Colorado, Boulder, CO, US
Colorado University
Joint Inst. for Lab. Astrophysics, Boulder, CO
Joint Institute for Laboratory Astrophysics, University of Colorado and National Institute of Standards and Technology, Boulder, CO 80309-0440, USA
JILA, University of Colorado, 440 UCB, Boulder, CO 80309, USA
Joint Institute for Laboratory Astrophysics, University of Colorado and National Bureau of Standards, Boulder, Colorado 80309 and Department of Astrophysical, Planetary, and Atmospheric Sciences, University of Colorado, Boulder, Colorado 80309
JILA, University of Colorado, Boulder, CO 80309-0440, USA
Joint Inst. for Laboratory Astrophysics, Boulder, CO
Colorado, University; Joint Institute for Laboratory Astrophysics, Boulder
Colorado Univ., Boulder, CO, US
JILA, University of Colorado, Boulder, Colorado 80309-0440, USA Joss Bland-Hawthorn is at the Anglo-Australian Observatory, PO Box 296, Epping, New South Wales 2121, Australia.
JILA
JILA, Boulder
Univ. of Colorado
JILA, University of Colorado, Boulder, CO
California, University, Berkeley, CA; Cambridge University, Cambridge, England
JILA, Campus Box 440,
3D FLASH simulations of AGN heating in clusters of galaxies
3D Simulations of Viscous Dissipation in the Intra-cluster Medium
3D simulations of viscous dissipation in the intracluster medium
A Critical Analysis of Ideal Magnetohydrodynamic Models for Crab-like Pulsar Winds
A Good Long Look at the Black Hole Candidates LMC X-1 and LMC X-3
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Profile ID: LFWR-SCP-P-28609