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Astronomers classify white dwarfs based on their spectral lines, which reveal the composition of their thin outer atmospheres. Spectral Type Primary Atmospheric Characteristics Hydrogen-rich atmosphere (strong Balmer absorption lines) DB Helium-rich atmosphere (neutral Helium lines) DO Ionized Helium-rich atmosphere (hot white dwarfs) DQ Carbon features present in the spectrum DZ To find the archives, users generally enter keywords
As the door hissed open to reveal the armored silhouettes of the law, Kaelen closed his eyes. In the darkness of his mind, he wasn't in a crumbling hive; he was on a green battlefield under a sun that would never set, rolling dice for the fate of a galaxy that was still young. In the darkness of his mind, he wasn't