Education Stars

1.Stars2. Temperature Hot = blue star(about 30,000 o ) Cool = red star(about 2500 o ) Sun = yellow star(about 6000 o ) 3. Constellation Orion 4. Brightness Apparent Magnitude(m)…

Documents Population Synthesis of Millisecond X-ray Pulsars

ar X iv :1 50 9. 05 02 7v 1 [a str o- ph .H E] 1 6 S ep 20 15 Mon. Not. R. Astron. Soc. 000, 1–12 () Printed 18 September 2015 (MN LATEX style file v2.2) Population Synthesis…

Documents Stellar Disruptions of Super Massive Black Holes Ron Caplan March 7, 2003.

Slide 1 Stellar Disruptions of Super Massive Black Holes Ron Caplan March 7, 2003 Slide 2 Outline Ron Caplan Outline Structure Accretion Disruption Flare Wind Remnants Observation…

Documents Star Formation Daniel Zajfman Department of Particle Physics Weizmann Institute of Science.

Star Formation Daniel Zajfman Department of Particle Physics Weizmann Institute of Science Stars Planets Galaxies Black holes Nebulae Red giants White dwarf Moons Supernovae…