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helium shell flash
subjectfact 
helium shell flashhas definition It has been shown that helium shell burning outside a degenerate core is unstable; the helium-burning shell does not generate energy at a constant rate but instead produces energy primarily during short flashes. During a flash, the region just outside the helium-burning shell becomes unstable to convection. The resultant mixing probably leads to the s-process as well as to the upward movement of carbon produced by helium burning.has source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press, 2001-09-27 09:29:43.0
is a kind of helium burning2001-09-27 09:29:43.0
helium burninghas duration 5 × 105 years2001-09-27 09:29:43.0
has optimum density 700 g/cm32001-09-27 09:29:43.0
requires minimum mass at star birth 0.5 solar masses2001-09-27 09:29:43.0
has optimum temperature 2 × 108 K2001-09-27 09:29:43.0
has part product carbon2001-09-27 09:29:43.0
has next higher temperature reaction carbon burning2001-09-27 09:29:43.0
has product carbon, oxygen2001-09-27 09:29:43.0
has reactant helium2001-09-27 09:29:43.0
exothermic fusion processliberates energy2001-09-27 09:29:41.0
fusionhas antonym fission2001-09-27 09:29:41.0
produces energy2001-09-27 09:29:41.0
has reaction probability2001-09-27 09:29:41.0
has catalyst2001-09-27 09:29:41.0
has minimum temperature2001-09-27 09:29:41.0
physical processhas domain physics2001-09-27 09:29:38.0

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