Low-mass stars are expected to become white dwarves.
A low mass star will become a white dwarf star, eventually this will cool to become a black dwarf. A high mass star (at least 8 times the mass of our Sun) will form a neutron star or a black hole, after a supernova event.
a low mass protostar is the begining formation of a low mass star. a low mass protostar is formed by a nebula (stellar nursery), like a cloud in space, where all stares come from. the definition of protostar is: a collection of gas, and dust who`s gravitational pull is causing it to collapse on itself & form a star. a LOW MASS protostar just has a LOWER MASS then a HIGH MASS protostar. Your Welcome:)
A high-mass star will use up its fuel faster than a low-mass one. Depending on the amount of mass that remains at the end of its life, it may convert to a neutron star, or to a black hole.
High mass.
A red gaint star is a luminous star of low or intermediate mass(0.5ms to 10ms). its
A white dwarf is the remnant of a low to medium mass star.
Helium. A low mass star does not have enough mass to generate the heat needed to fuse helium.
After a low-mass or medium-mass star dies, it will typically leave behind a remnant called a white dwarf. A white dwarf is a dense, Earth-sized core made primarily of carbon and oxygen. It gradually cools and fades over billions of years.
The Sun is a medium mass star in main sequence.
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A low mass star begins as the helium fuses into carbon and the core collapses. The outer layer of the star are expelled and form a new planetary nebula. The core remains as a white dwarf and cooled to become a black dwarf.
Not necessarily. A white dwarf is simply the remains of a low to medium mass star that has died. A red dwarf is a low mass star. Since red dwarfs last longer than medium mass stars, one could easily be older than a white dwarf.