Hype williams
The life cycle of a star
A Brief History and Research of the Supernova Cas A
Detection of highvelocity_material_from_the_win_wind_collision_zone_of_eta_carinae
Stellar Evolution II. The Upper End of the Main Sequence: How massive can a star get? Larger clouds of gas (GMCs) tend to fragment into smaller ones before.
INAF The advanced evolutionary phases of the massive stars and their explosive yields Alessandro Chieffi Istituto Nazionale di AstroFisica (Istituto di.
Steve B. Howell (NOAO) Don Hoard (Spitzer Science Center Bob Stencel (U. of Denver)
1 Science and the VO – Overview and Discussion Dave De Young NVO Project Scientist NOAO NVOSS Santa Fe September 2008.
1 Science and the NVO – Overview and Discussion Dave De Young NVO Project Scientist NOAO NVOSS Aspen September 2006.
An update of results from the Princeton MRI Experiment Mark Nornberg Contributors: E. Schartman, H. Ji, A. Roach, W. Liu, and Jeremy Goodman CMSO General.
What determines Luminosity? Stephans law: Power radiated depends on Temp to the 4 th power! Stephans law: Power radiated depends on Temp to the 4 th power!
Reviewing some of the concepts covered in class this year.
