'Fe core' diaporamas de présentation

APCTP-YITP@kyoto

APCTP-YITP@kyoto. Spin of Stellar Mass Black Holes: Key to Gamma-ray Bursts and Hypernovae. in collaboration with G.E. Brown, R.A.M.J. Wijers, et al. ApJ 575, 996 (2002) ApJ 671, L41 (2007) astro-ph/0612461 arXiv:0801.0477. Chang-Hwan Lee @. Contents. Motivations. GRB.

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Post-Main Sequence Evolution of Massive Stars

Post-Main Sequence Evolution of Massive Stars. Stars of more than 8 solar masses leave behind neutron stars and black holes and typically explode as supernovae. But first, NOVAE from WDs. Back to binary star evolution: More massive star leaves MS first, becomes RG, then WD

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PRESUPERNOVA EVOLUTION AND EXPLOSION OF MASSIVE STARS: CHALLENGES OF THE NEXT CENTURY

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Different kinds of Stars

Different kinds of Stars. In an Hertzsprung-Russell Diagram (or H-R diagram or color-magnitude diagram) each star is plotted as a point. The horizontal axis of the H-R diagram can be any of several measures of surface temperture:.

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The structure and evolution of stars

The structure and evolution of stars. Lecture13: Supernovae - deaths of massive stars. Complete notes available online: http://star.pst.qub.ac.uk/~sjs/teaching.html. Learning Outcomes. In these final two lectures the student will learn about the following issues: What is a supernova

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The structure and evolution of stars

The structure and evolution of stars. Lecture13: Supernovae - deaths of massive stars. Complete notes available online: http://star.pst.qub.ac.uk/~sjs/teaching.html. Learning Outcomes. In these final two lectures the student will learn about the following issues: What is a supernova

327 views • 21 slides

The structure and evolution of stars

The structure and evolution of stars. Lecture13: Supernovae - deaths of massive stars. Complete notes available online: http://star.pst.qub.ac.uk/~sjs/teaching.html. Learning Outcomes. In these final two lectures the student will learn about the following issues: What is a supernova

216 views • 21 slides