Stellar Death Flashcards
(Outcome of stellar evolution) the star explodes, ejecting all of its matter into interstellar medium
Nothing/recycling
(Outcome of stellar evolution) degenerate core stays and slowly cools and fade
White dwarf
(Outcome of stellar evolution) extremely compact core stays behind when star explodes - will eventually fade
Neutron star
(Outcome of stellar evolution) singularity/point of infinite curvature left behind when star goes supernova
Black hole
(Supernovae) shows no hydrogen in their spectrum
Type I
(Supernovae) strong hydrogen in spectrum
Type II
(Supernovae) strong silicon
Type Ia
(Supernovae) He rich
Type Ib
(Supernovae) He poor
Type Ic
Luminosity/magnitude vs. time
Lightcurve
Star begins to collapse once core (degenerate) is iron (Fe) and no white dwarf or planetary nebula is left
Core-collapse supernovae
Photons break apart heavy nuclei
Photodisintegration
Escaping neutrinos cool the star as it collapses
Proto-neutron star
What powers supernovae
gravitational energy released from core collapse
Compressed neutrons will exert
Neutron degeneracy pressure