Keywords
relevant to the
SNe Ia (Type Ia supernovae)
:
accretion disk
,
binary stars
,
compact remnants
(
white dwarfs
,
neutron stars
,
black holes
),
convection
,
double-degenerate scenario
,
gigayears (Gyr)
,
globular clusters
,
gravitational potential energy
,
gravity
,
heat energy
,
Hertzsprung-Russell (HR) diagram
,
hydrogen (H)
,
hydrogen burning
,
kinetic energy
,
luminosity
,
luminosity class
,
main sequence
,
main-sequence stars
,
metalliticity
,
metals
,
multiple star systems
,
neutrinos (ν)
(
electron neutrinos (ν_e)
),
neutrons (n)
,
neutron stars
,
nuclear binding energy
,
nuclear burning
,
nuclear fusion
,
nuclear physics
,
nuclear reactions
,
nuclei
,
OBAFGKM stellar classification system
,
open star clusters
,
photons
,
photosphere
,
photospheric temperature
(
color temperature
,
effective temperature
),
protons (p+)
,
radiative transfer
,
rest mass
,
Roche lobe
,
solar mass M_☉ = 1.98855(25)*10**30 kg
,
stars
,
star clusters
(
open star clusters
,
globular clusters
),
single-degenerate scenario
,
SN 1006 (SNe Ia probably)
,
SN 1572 (AKA Tycho's supernova, SNe Ia)
,
SN 1604 (AKA Kepler's supernova, SNe Ia)
SNe Ia (Type Ia supernovae)
),
SNe Ia scenarios
(
single-degenerate scenario
,
double-degenerate scenario
,
SNe Iax (Type Iax)
),
stellar evolution
,
stellar mass
,
stellar populations
(
Population I stars
,
Population II stars
,
Population III stars
),
stellar rotation
,
stellar winds
,
strong nuclear force
,
supernovae
(
core collapse supernovae
,
SNe Ia (Type Ia supernovae)
),
supernova remnants
,
weak nuclear force
,
white dwarfs
,
Wien's law
,
zero-age main sequence (ZAMS)
.
Local file:
local link: sne_ia_keywords.html
.
File:
Star file
:
sne_ia_keywords.html
.