Temperature |
Luminosity |
|
Harvard |
M |
1: |
3350 K |
Harvard spectral value is 1: with class Harvard spectral class M with effective temperature [2000, 3500] ; absorptions [Metals,
TiO]
|
Yerkes |
V |
Yerkes spectral luminosity with class V: main-sequence star |
e |
~ |
COBREX simplification = M1 ~
Temperature |
Harvard |
M |
1 |
3350 K |
Harvard spectral value is 1 with class Harvard spectral class M with effective temperature [2000, 3500] ; absorptions [Metals,
TiO]
|
~ |
Ref: An Encoding System to Represent Stellar Spectral Classes in Archival Databases and Catalogs
Version 1.4