Astronomical Solutions to Galactic Dark Matter Will Sutherland Institute of Astronomy, Cambridge.
Galaxies. Galactic Morphology Interacting Galaxies "Active" Galaxies.
Unstructured grids for Astrophysics Gas dynamics and radiative transfer C.P. Dullemond Max Planck Institute for Astronomy Heidelberg, Germany.
Mu Cephei name was known as “Garnet Star” because of it’s deep red color.
YOUKO
Ch. 9 – The Lives of Stars from Birth through Middle Age Second part The evolution of stars on the main sequence.
Neutron Stars Chandrasekhar limit on white dwarf mass Supernova explosions –Formation of elements (R, S process) –Neutron stars –Pulsars Formation of X-Ray.
Ch. 9 The Lives of Stars from Birth through Middle Age The Cone Nebula.
RHESSI and the solar radius H.S. Hudson, M.D. Fivian & H.J. Zahid Space Sciences Lab, UC Berkeley First report of our semi-intentional optical limb astrometry.
Solar Science Workshop 6/8/05 An Introduction to the Physics of Our Star: The Sun Distance from Earth –1 AU Travel time for Light to Earth –About 8 minutes.
Characteristics of Stars Analyze how stars are classified based on their physical characteristics.
December 14, 2007, AGU Fall Meeting, San Francisco, (SH53A-1076)1 Solar Shape Measurements from RHESSI ‘A Large Excess Oblateness ?’ M.D. Fivian, H.S.
