ବହୁତ ବଡ ବ୍ୟାସ ଏବଂ ନିମ୍ନ ଘନତା ସହିତ ଏକ ଉଜ୍ଜ୍ୱଳ ତାରକା |,

Noun:

ରାକ୍ଷସ,

supergiant's Usage Examples:

8) is a blue supergiant O-type star in the tail of dwarf irregular galaxy IC 3418.

It is a yellow-white supergiant that pulsates between spectral types F6Ib-II and G1Ib-II.

An OH/IR star is an asymptotic giant branch (AGB) or a red supergiant or hypergiant (RSG or RHG) star that shows strong OH maser emission and is unusually.

Some models suggest that LBVs are a stage in the evolution of very massive stars required for them to shed excess mass, whereas others require that most of the mass is lost at an earlier cool-supergiant stage.

combined mass does not exceed the Chandrasekhar limit, the helium will accrete onto the C-O dwarf and ignite to form a supergiant.

UY Sct is a dust-enshrouded bright red supergiant and is classified as a semiregular variable with.

"The mass-loss rates of red supergiants and the de Jager prescription".

("dwarfs") Subgiants Giants Bright giants Supergiants Hypergiants absolute magni- tude (MV) Red supergiants (RSGs) are stars with a supergiant luminosity.

Both types of star have luminous and unstable photospheres at this stage of their lives and often have the spectra of supergiants.

The recorded spectrum of the optical light echo proved the supernova was of Type IIb, meaning it resulted from the internal collapse and violent explosion of a massive star, most probably a red supergiant with a helium core which had lost almost all of its hydrogen envelope.

oxygen-rich red supergiant star, a place where substances containing metals or hydroxides are thought to be rare.

luminosities comparable to supergiants.

Synonyms:

star,

Antonyms:

minor, lack,