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physical object > natural object > celestial body > star > early star > white dwarf |
white dwarf comparison table |
Subject | has surface temperature | is part of | is a kind of | has radiu | is an instance of | has mass | has definition | has distance | has density |
---|---|---|---|---|---|---|---|---|---|
DA white dwarf | greater than 1000 Kelvin | white dwarf | greater than 0.08 the sun's mass | only strong hydrogen lines present | |||||
DB white dwarf | greater than 1000 Kelvin | white dwarf | greater than 0.08 the sun's mass | only strong helium lines present | |||||
DC white dwarf | greater than 1000 Kelvin | white dwarf | greater than 0.08 the sun's mass | continuous spectrum, no lines clearly visible | |||||
DO white dwarf | greater than 1000 Kelvin | white dwarf | greater than 0.08 the sun's mass | both He and H lines present | |||||
DQ white dwarf | greater than 1000 Kelvin | white dwarf | greater than 0.08 the sun's mass | carbon lines (atomic or molecular) present. | |||||
DZ white dwarf | greater than 1000 Kelvin | white dwarf | greater than 0.08 the sun's mass | no He nor H lines, but metallic lines present | |||||
Omicron2 Eridani | greater than 1000 Kelvin | Eridanus | white dwarf | greater than 0.08 the sun's mass | A triple star that was the first white dwarf ever discovered. | 16 light-years | |||
Sirius B | Teff = 32000 K | Canis Major | 0.03 solar radii | white dwarf | 1 solar mass | Companion of Sirius, a white dwarf. | |||
van Maanen's star | greater than 1000 Kelvin | white dwarf | greater than 0.08 the sun's mass | 4 pc | 4 × 105 g cm-3 |
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