DOCUMENT RESOURCES FOR EVERYONE
Documents tagged
Documents 1 OPTIMIZATION OF ACTINIDE QUANTIFICATION BY ELECTRON PROBE MICROANALYSIS Aurélien Moy Claude...

Slide 11 OPTIMIZATION OF ACTINIDE QUANTIFICATION BY ELECTRON PROBE MICROANALYSIS Aurélien Moy Claude Merlet (UM2/GM) Xavier Llovet (Universitat de Barcelona/CCiTUB) Olivier…

Documents The evolution of SMBH from Hard X-ray surveys Andrea Comastri (INAF – Osservatorio di Bologna –....

Slide 1The evolution of SMBH from Hard X-ray surveys Andrea Comastri (INAF – Osservatorio di Bologna – Italy) The XRB as a tracer of SMBH mass density Hard X-ray surveys:…

Documents RevModPhys.76.1143

The physics of gamma-ray bursts Tsvi Piran* Racah Institute for Physics, The Hebrew University, Jerusalem, 91904, Israel ~Published 28 January 2005! Gamma-ray bursts sGRB’sd,…

Documents Electron Beam Analysis (EPMA, SEM-EDS) Warren Straszheim, PhD EPMA, Ames Lab, 227 Wilhelm SEM-EDS,.....

Slide 1Electron Beam Analysis (EPMA, SEM-EDS) Warren Straszheim, PhD EPMA, Ames Lab, 227 Wilhelm SEM-EDS, MARL, 23 Town Engineering [email protected] 515-294-8187 [email protected]

Documents The Sun – Our Star Chapter 7:. General Properties Average star Absolute visual magnitude = 4.83...

Slide 1 The Sun – Our Star Chapter 7: Slide 2 General Properties Average star Absolute visual magnitude = 4.83 (magnitude if it were at a distance of 32.6 light years)…

Documents The Sun – Our Star Chapter 8. The preceding chapter described how we can get information from a...

Slide 1 The Sun – Our Star Chapter 8 Slide 2 The preceding chapter described how we can get information from a spectrum. In this chapter, we apply these techniques to the…

Documents Unit 5: Sun and Star formation. General Properties Average star Absolute visual magnitude = 4.83...

Slide 1 unit 5: Sun and Star formation Slide 2 General Properties Average star Absolute visual magnitude = 4.83 (magnitude if it were at a distance of 32.6 light years) Central…

Documents Analysis of Doppler-Broadened X-ray Emission Line Profiles from Hot Stars David Cohen - Swarthmore.....

Slide 1 Analysis of Doppler-Broadened X-ray Emission Line Profiles from Hot Stars David Cohen - Swarthmore College with Roban Kramer - Swarthmore College Stanley Owocki -…

Documents High-resolution X-ray spectroscopy with microcalorimeters L. Piro Some key scientific drivers:...

Slide 1 High-resolution X-ray spectroscopy with microcalorimeters L. Piro Some key scientific drivers: –GRB engine and progenitors: X-ray lines and absorption features…

Documents The Sun – Our Star

PowerPoint Presentation - The Milky Way The Sun – Our Star Chapter 8 The preceding chapter described how we can get information from a spectrum. In this chapter, we apply…