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- W74607544 abstract "Since some of the earliest evolutionary calculations it has been found that post main sequence stars become red giants (e.g. Sandage and Schwarzschild, 1952). However the exact physical processes that lead to and determine the rate of redward evolution are not completely understood." @default.
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- W74607544 date "1984-01-01" @default.
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- W74607544 title "The role of the radiation pressure gradient in giant and supergiant star evolution" @default.
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- W74607544 doi "https://doi.org/10.1017/s007418090003059x" @default.
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