Pulsars High Energy Astrophysics [email protected]
Extra-Solar Planets Planetary Physics Summer Term 2004 Lecture 10.
The multi-wavelength context of the future gamma-ray instruments: X-rays T. Dotani 1), A. Bamba 2), T. Fujinaga 3,1) 1) ISAS/JAXA 2) Aoyama Gakuin Univ.
Neutron Stars. Gradual compression of a stellar iron core trans. [g cm -3 ] CompositionDegen. pressure Remarks Iron nuclei; nonrel. free e - nonrel.
Lives of Stars. A star is born… All stars begin their lives as NEBULAS, large clouds of gas and dust spread out in an immense volume. A STAR, on the.
Review for Quiz 2. Outline of Part 2 Properties of Stars Distances, luminosities, spectral types, temperatures, sizes Binary stars, methods of estimating.
Neutron Stars and Black Holes Please press “1” to test your transmitter.
Presented by: Jorge A Campos. Description part of NASA's fleet of "Great Observatories" including: the Hubble Space Telescope the Spitizer Space Telescope.
Life Cycle of a Star Based on Mass of Star. All Stars – Stage 1-Nebula Gravity main force, pulls cloud INWARD. Temperature = INCREASES Gravity based on.
Neutron Stars and Black Holes Chapter 14. The preceding chapters have traced the story of stars from their birth as clouds of gas in the interstellar.
What's in our galaxy?. Emission Nebulae Spectra consist of emission lines Are hot, ionised hydrogen plasma (plus a few other elements) where stars are.
Compact Objects Astronomy 315 Professor Lee Carkner Lecture 15.