emamajek on 27-Aug-2017 05:58:51 GMT about HD 79211
GJ 338 B is considered a spectral standard star of type "K7V" by
1991ApJS...77..417K
and "K7.0V" by
2002AJ....123.2002H
.
Kirkpatrick+1991 notes that GJ 338 B actually has a slightly earlier spectral type (K7V) than the primary GJ 338 A (M0V), where A and B are designated by Gliese+ 1991. Henry+2002 corroborates this, with the primary GJ 338 A (M0.0V) listed at (J2000) 09:14:22.8 +52:41:12, and the secondary GJ 338 B (K7.0V) listed at (J2000) 09:14:24.7 +52:41:11. So the type currently listed (M0V) appears to be a typo, but correct for the primary.
This is somewhat confusing as other works have determined spectroscopic Teffs where A is indeed marginally hotter than B (e.g.
2009ApJ...704..975J
,
2014MNRAS.443.2561G
,
2015ApJ...800...85N
), as expected for its slightly brighter magnitude.
The original catalog that sets A and B (Gliese+1991) confirms that "A" is at lower RA, brighter V mag, and bluer B-V, U-B, and R-I colors compared to "B".
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