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Spectroscopic Analysis of Hydrogen Emission Lines and Velocity Shifts

DESCRIPTION

This study investigates the hydrogen emission lines observed in a stellar spectrum. We analyze three distinct velocity shifts of hydrogen (Ha) at 6580 Å, 6563 Å, and 6510 Å, corresponding to velocities of -3000 km/s, 0 km/s, and +3000 km/s, respectively. These findings provide insight into the kinematic properties of the observed object, revealing information about its motion relative to the observer. The spectral data contributes to our understanding of stellar dynamics and the physical processes within astronomical environments.

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Spectroscopic Analysis of Hydrogen Emission Lines and Velocity Shifts

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  1. Vr = -3000 km/s l Ha ≈ 6580 Å Vr = 0 km/s 3000 km/s l Ha ≈ 6563 Å Vr = + 3000 km/s l Ha ≈ 6510 Å observateur

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