lowtointermediatemass

Lowtointermediatemass is a term used in astrophysics to describe a range of stellar masses. Stars are broadly categorized by their mass, which dictates their temperature, luminosity, lifespan, and eventual fate. The low-to-intermediate mass range typically encompasses stars that are less massive than stars like our Sun, but also less massive than the much larger and more luminous stars.

This mass range is significant because it includes many common types of stars and plays a crucial role in galactic evolution. Stars in this category are often the most numerous in the universe. Their evolutionary paths are distinct from both the very low-mass stars (red dwarfs) and the high-mass stars.

The specific boundaries of the "low-to-intermediate" range can sometimes vary slightly depending on the context or the specific stellar population being studied. However, it generally refers to stars with masses roughly between 0.5 and 8 times the mass of our Sun. Stars in this range fuse hydrogen into helium in their cores for the majority of their lives. Their subsequent evolution involves stages like red giants and, for some, the formation of white dwarfs. The study of these stars helps astronomers understand the life cycles of a vast number of celestial objects.