Line Profiles Note - Figure obtained from lsa.atnos/SAElp05.htmlsa.atnos/SAElp05.htm.
Chapter 11 Stars Properties of Stars Classifying Stars –Hertzsprung-Russel (H-R) Diagram Star Clusters –Open and Globular Clusters.
Science project 3
19730005065_1973005065
Astrophysical applications of gravitational microlensing By Shude Mao Ziang Yan Department of Physics,Tsinghua.
The information contained in light : A basic introduction to astronomical spectroscopy (stars, galaxies,QSO) National Astronomical Observatories of China,
Wavelength flux Spectral energy distributions of bright stars can be used to derive effective temperatures Ay 123 Lecture I - Physical Properties.
PHYS 3380 - Astronomy Homework Set #5 10/01/14 Due 10/08/14 Chapter 7 Review questions 4 and 5 Problems 1, 5, and 7 Learning to Look 1 Extra Problem 1.
Interstellar Matter and Star Formation Chapter 13 Courtesy of Wolfgang Brandner (JPL/IPAC), Eva K. Grebel (Univ. Washington), You- Hua Chu (Univ. of Illinois,
Model Photospheres
The DACs and SACs effects from stars to Quasars. Some first general notices
Publications Based on SALT data Poland
