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- W4231331765 abstract "We present spectroscopic distances for 22 central stars of planetary nebulae. These distances have been determined using information provided by our non-LTE model atmosphere analyses of the stellar H and He absorption line profiles. In this way, no assumptions about nebular properties are necessary. Our spectroscopic distances turn out to be larger than many other frequently cited values. We show that our distances are not in contradiction with the available information about the interstellar extinction, and we describe additional evidence supporting them." @default.
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- W4231331765 date "1989-01-01" @default.
- W4231331765 modified "2023-09-26" @default.
- W4231331765 title "Spectroscopic Distances to Central Stars of Planetary Nebulae" @default.
- W4231331765 cites W2026110424 @default.
- W4231331765 doi "https://doi.org/10.1017/s0074180900137751" @default.
- W4231331765 hasPublicationYear "1989" @default.
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