The top documents tagged [xray lines]

1 OPTIMIZATION OF ACTINIDE QUANTIFICATION BY ELECTRON PROBE MICROANALYSIS Aurélien Moy Claude Merlet (UM2/GM) Xavier Llovet (Universitat de Barcelona/CCiTUB)
Documents 1 OPTIMIZATION OF ACTINIDE QUANTIFICATION BY ELECTRON PROBE MICROANALYSIS Aurélien Moy Claude Merlet (UM2/GM) Xavier Llovet (Universitat de Barcelona/CCiTUB)

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The 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
Documents The 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

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AST 4.6 PPT
Documents AST 4.6 PPT

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RevModPhys.76.1143
Documents RevModPhys.76.1143

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Electron Beam Analysis (EPMA, SEM-EDS) Warren Straszheim, PhD EPMA, Ames Lab, 227 Wilhelm SEM-EDS, MARL, 23 Town Engineering wesaia@iastate.edu 515-294-8187
Documents Electron Beam Analysis (EPMA, SEM-EDS) Warren Straszheim, PhD EPMA, Ames Lab, 227 Wilhelm SEM-EDS, MARL, 23 Town Engineering [email protected] 515-294-8187

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Unit 5: Sun and Star formation. General Properties Average star Absolute visual magnitude = 4.83 (magnitude if it were at a distance of 32.6 light years)
Documents Unit 5: Sun and Star formation. General Properties Average star Absolute visual magnitude = 4.83 (magnitude if it were at a distance of 32.6 light years)

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

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

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

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

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The Sun – Our Star
Documents The Sun – Our Star

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The Sun – Our Star
Documents The Sun – Our Star

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