Its outer hydrogen envelope becomes more loosely bound and vulnerable to gravitational stripping, or a type of stellar cannibalism, by the nearby companion star.
Not exact matches
Eventually, Stars Aa and Ab will lose much of their current mass, from intensified stellar winds that eventually puff out their
outer gas
envelopes of
hydrogen and helium (and lesser amounts of higher elements such as carbon and oxygen) into interstellar space as planetary nebulae.
Information about the ang... ▽ More When the core
hydrogen is exhausted during stellar evolution, the central region of a star contracts and the
outer envelope expands and cools, giving rise to a red giant, in which convection occupies a large fraction of the star.
Abstract: When the core
hydrogen is exhausted during stellar evolution, the central region of a star contracts and the
outer envelope expands and cools, giving rise to a red giant, in which convection occupies a large fraction of the star.