Figure 7 from Data-driven Spectroscopic Estimates of Absolute Magnitude, Distance, and Binarity: Method and Catalog of 16,002 O- and B-type Stars from LAMOST

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF

Data-driven Spectroscopic Estimates of Absolute Magnitude, Distance, and Binarity: Method and Catalog of 16,002 O- and B-type Stars from LAMOST

Authors: Mao-Sheng Xiang, Hans-Walter Rix, Yuan-Sen Ting, Eleonora Zari, Kareem El-Badry, Hai-Bo Yuan, and Wen-Yuan Cui

2021 The Astrophysical Journal Supplement Series 253 22.

Provider: AAS Journals

Caption: Figure 7.

Differences between spectroscopic ﹩{M}_{K{\rm{s}}}﹩ and geometric ﹩{M}_{K{\rm{s}}}﹩ as a function of stellar parameters. Only results for single stars are shown. The solid lines delineate the median and standard deviation as a function of stellar parameters.

Other Images in This Article

Copyright and Terms & Conditions