PX269 Galaxies Part 2: Our Galaxy, the Milky Way 2.1 Components and Structure PX269 Galaxies.
Development of a depository in an analytical facility –– a sample-preservation mission Tak Kunihiro, Y. Yachi, H. Kitagawa, and E. Nakamura Pheasant Memorial.
Ch.4. Broad Line Region broad lines are important to understand AGN structure for at least two reasons: 1) BLR motions are almost certainly determined.
AFM-Raman and Tip Enhanced Raman studies of modern nanostructures Pavel Dorozhkin, Alexey Shchekin, Victor Bykov NT-MDT Co., Build. 167, Zelenograd Moscow,
Chandra Calibration Status ACIS 1.Gain correction files for epochs 30, 31 and 32 were released in CALDB 3.4.1 (Sept 2007), 3.4.2 (Dec. 2007) and 3.4.3.
Microphysics of the radiative transfer. Numerical integration of RT in a simplest case Local Thermodynamical Equilibrium (LTE, all microprocesses are.
Magnetic Fields at Mt. Wilson and MDI. The 150-foot Tower Spectrograph Measures 12 line pairs simultaneously The long-term program uses 5250. The full.
Finding Photospheric Flows with I+LCT or,“Everything you always wanted to know about velocity at the photosphere, but were afraid to ask.” B. T. Welsch,
Spring School of Spectroscopic Data Analyses 8-12 April 2013 Astronomical Institute of the University of Wroclaw Wroclaw, Poland.
SHINE 2008
AFM-Raman and Tip Enhanced Raman studies of modern nanostructures
Measuring the black hole spin of GX 339-4: A systematic look at its very high and low/hard state. Rubens Reis Institute of Astronomy - Cambridge In collaboration.
