Calculations of resonance line profiles from thin layers in rotating accretion disks show symmetric shapes for continuous or double-spot atom distributions and asymmetric shapes for single rotating spots, varying with rotation-to-Doppler velocity ratio and electron-to-atom density ratio.
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Resonance line in rotating accretion disc
Calculations of resonance line profiles from thin layers in rotating accretion disks show symmetric shapes for continuous or double-spot atom distributions and asymmetric shapes for single rotating spots, varying with rotation-to-Doppler velocity ratio and electron-to-atom density ratio.