Spectrophotometry of white dwarfs as observed at high signal-to-noise ratio. II

• 1 September 1990
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 360, 662-684
• https://doi.org/10.1086/169153

Abstract

Keywords

• SIGNAL TO NOISE RATIOS
• STELLAR SPECTROPHOTOMETRY
• WHITE DWARF STARS
• BALMER SERIES
• CARBON
• CHARGE COUPLED DEVICES
• H ALPHA LINE
• SPECTRAL ENERGY DISTRIBUTION
• SPECTRAL LINE WIDTH