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at which point the density and temperature will become so high that the fusion of helium into carbon will beginleadingto a helium flash
the ignition of helium fusion in a core that contains degenerate electrons(passive) is caused byPresent A helium flash
nuclear fusion similar to the process by whichcreatesa helium flash
the pressure ... high enough in the hydrogen layerto triggerthe helium flash
Degenerate gas core 10 8 K Helium fusion through triple alphacausesa helium flash
the explosive ignition of helium in the electron - degenerate core of a low mass ( $ < 2M_{\odot}$ ) star(passive) is caused byThe helium flash
the addition of helium to the core by shell hydrogen burning ... a rapid burst of helium burning in the core , after which the star will commence a brief period of helium burning before beginning another ascent of the red giant branchwill causea helium flash
When the Sun trust in the red giant stage initiates hydrogen fusion in the layer of hydrogen surrounding the corecreatingthe helium flash
that the fusion of helium into carbon will start outleadingto a helium flash
the star burns uncontrollably for a few hours ... the star burns uncontrollably for a few hourscausesa Helium Flash
This increase in tempcausesa Helium Flash
Energy pressureresultsin a helium flash
the critical masstriggersthe helium flash
If the companion is " an evolving star " , then why would enough helium fall onto the white dwarfto causea helium flash
M ☉ yr–1 , the accreted helium ignites unstablyresultingin a helium flash
Msol / yr , the accreted helium ignites unstablyresultingin a helium flash
what halts their evolutioncausesthe helium flash
For accretion rates < 10{sup -6 } M { sub sun } yr{sup -1 } , the accreted helium ignites unstablyresultingin a helium flash
a series of different waves moving out through the starwill causea series of different waves moving out through the star
to a supernova explosion and collapse of star remnants increase in temperature and pressure leading to reignition and eventual formation of a Cepheid variable exhaustion of all nuclear fuel and collapse of the star into a white dwarf pressure increase leading to ignition of elements heavier than iron temperature rise leading to a supernova explosion and collapse of the remaining matter to form a brown dwarf Which line in the table best documents the events at the end of the life cycle of most stars that are ten or more times more massive than the sunleadingto a supernova explosion and collapse of star remnants increase in temperature and pressure leading to reignition and eventual formation of a Cepheid variable exhaustion of all nuclear fuel and collapse of the star into a white dwarf pressure increase leading to ignition of elements heavier than iron temperature rise leading to a supernova explosion and collapse of the remaining matter to form a brown dwarf Which line in the table best documents the events at the end of the life cycle of most stars that are ten or more times more massive than the sun
up a continuing state of following helium flares ad infinitumsetsup a continuing state of following helium flares ad infinitum
and consume most of the Hewould be triggeredand consume most of the He
The solar(passive) is setThe solar
this event ... considerably longer than the equivalent evolutionary period in the Blöcker ( 1995 ) modelscausedthis event ... considerably longer than the equivalent evolutionary period in the Blöcker ( 1995 ) models
The discontinuity at 11 Gyr(passive) is caused byThe discontinuity at 11 Gyr
in a white dwarf supernova by compressing the core enough to pass the Chandrasekhar limit even though it does n't have enough mass : https://arxiv.orgcould resultin a white dwarf supernova by compressing the core enough to pass the Chandrasekhar limit even though it does n't have enough mass : https://arxiv.org