Otros recursos de White, Richard L.
| Resultados 1 - 10 de 189 de White, Richard L.. (0,09 segundos) |
Documentos:

1. (100%)
On-board image compression for the HST Advanced Camera for Surveys
- Richard L. White
The Wide Field Camera in the Advanced Camera for Surveys (ACS) produces very large 4096
×
4096 pixel ...
(ps) - 31-mar-2009

2. (100%)
Hubble Space Telescope: High speed photometer instrument handbook. Version 2.0
- White, Richard L.
This manual is a guide for astronomers who intend to use the High Speed Photometer (HSP), one of the ...
- 28-abr-2009

3. (100%)
High-performance compression of astronomical images
- White, Richard L.
Astronomical images have some rather unusual characteristics that make many existing image compressi ...
- 30-abr-2009

4. (100%)
Phase space simulation of collisionless stellar systems on the massively parallel processor
- White, Richard L.
A numerical technique for solving the collisionless Boltzmann equation describing the time evolution ...
- 09-jun-2009

5. (100%)
Gamma Ray Emission from Chaotic Winds of Massive Stars
- White, Richard L.
The purpose of this proposal was to search for gamma-ray emission from the winds of hot, massive sta ...
- 10-jun-2009

6. (88%)
Nonthermal radio emission from hot star winds: Its origin and physical implications
- Chen, Wan; White, Richard L.
Nonthermal radio emission has been observed from some of the most luminous hot star winds. It is und ...
- 29-abr-2009

7. (88%)
Particle acceleration, X-rays, and gamma-rays from winds
- White, Richard L.; Chen, Wan
The instability of the line-driven winds of hot stars leads to the formation of strong shocks. These ...
- 29-abr-2009

8. (88%)
Theory and Observations of Non-Thermal Phenomena in Hot Massive Binaries
- White, Richard L.; Chen, Wan
The shock between the colliding winds in binary systems containing two massive stars accelerates par ...
- 30-abr-2009

9. (88%)
Nonthermal Radio Emission from Hot Star Winds: Its Origin and Physical Implications
- Chen, Wan; White, Richard L.
Nonthermal radio emission has been observed from some of the most luminous hot star winds. It is und ...
- 04-may-2009

10. (88%)
Particle Acceleration, X-Rays, and Gamma-Rays From Winds
- White, Richard L.; Chen, Wan
The instability of the line-driven winds of hot stars leads to the formation of strong shocks. These ...
- 05-may-2009
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