Noun:

শ্বেতবামন,

white dwarf's Usage Examples:

A white dwarf, also called a degenerate dwarf, is a stellar core remnant composed mostly of electron-degenerate matter.

A white dwarf is very dense: Its.

one day, the white dwarf is close enough to its companion star to start drawing accreted matter onto the surface of the white dwarf, which creates a dense.

referred to as a dwarf star, this class of star may also be termed a yellow-white dwarf (not to be confused with white dwarfs, a possible final stage of stellar.

which one of the stars is a white dwarf.

The other star can be anything from a giant star to an even smaller white dwarf.

specifically a white dwarf that has cooled sufficiently that it no longer emits significant heat or light.

Because the time required for a white dwarf to reach.

(also known as WD 2354−211) is a white dwarf star located 65 pc (212 ly) away from the Earth.

It is a very faint white dwarf, with an apparent visual magnitude.

which are currently known to fit these conditions SDSS J1228+1040, A white dwarf with disk of debris.

components; a white dwarf primary, and a mass transferring secondary.

The stars are so close to each other that the gravity of the white dwarf distorts the.

It was one of the shortest-period detached binary white dwarf systems known in 2011 They are separated from each other by only 32%.

Sun has exhausted its nuclear fuel, its core collapses into a dense white dwarf and the outer layers are expelled as a planetary nebula.

The winter white dwarf hamster (Phodopus sungorus), also known as the Russian dwarf hamster, Djungarian hamster, striped dwarf hamster, Siberian hamster.

GD 40 is a white dwarf in the constellation Cetus.

believed that the white dwarf component of a symbiotic nova remains below the Chandrasekhar limit, so that it remains a white dwarf after its outburst.

BPM 37093 (V886 Centauri) is a variable white dwarf star of the DAV, or ZZ Ceti, type, with a hydrogen atmosphere and an unusually high mass of approximately.

201563164) is a white dwarf approximately 570 light-years (170 pc) from Earth in the constellation of Virgo.

It is the first white dwarf to be observed.

the less massive to the more massive white dwarf.

After it loses most of its mass, the less massive white dwarf may approach planetary mass.

degenerate star (white dwarf) of spectral class DQP9.

G 240-72 is the seventh closest white dwarf (after Sirius B, Procyon.

Synonyms:

white dwarf star; star;

Antonyms:

minor; lack;