Obj(BS/HD) | Sp. type |
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K | mag | ![]() |
||
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K5+III | 3874 | -1.7 ![]() |
1.5 ![]() |
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M0.5III | 3790 | -2.2 ![]() |
1.6 ![]() |
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M1III | 3812 | -2.2 ![]() |
1.7 ![]() |
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M1.5IIIa | 3909 | -3.2 ![]() |
3.6 ![]() |
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M2.5III | 3596 | -3.4 ![]() |
2.2 ![]() |
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M2.5III | 3852 | -3.4 ![]() |
3.7 ![]() |
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M2.5II-III | 3603 | -3.3 ![]() |
2.2 ![]() |
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M3+IIIa | 3712 | -2.9 ![]() |
2.0 ![]() |
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M3III | 3643 | -3.3 ![]() |
2.3 ![]() |
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M3III | 3643 | -2.4 ![]() |
1.4 ![]() |
10 Dra (5226) | M3.5III | 3730 | -2.9 ![]() |
2.1 ![]() |
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M4II | 3523 | -4.1 ![]() |
3.2 ![]() |
BS6861 (6861) | M4 | 3600 | -5.2 ![]() |
6.3 ![]() |
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M4II | 3420 | -5.5 ![]() |
5.5 ![]() |
RR UMi (5589) | M4.5III | 3397 | -3.4 ![]() |
1.6 ![]() |
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M5Ib-II | 3293 | -5.8 ![]() |
5.0 ![]() |
OP Her (6702) | M5II | 3325 | -4.4 ![]() |
2.3 ![]() |
XY Lyr (7009) | M5II | 3300 | -5.1 ![]() |
3.7 ![]() |
R Lyr (7157) | M5III | 3313 | -4.3 ![]() |
2.1 ![]() |
RZ Ari (867) | M6III | 3341 | -3.5 ![]() |
1.5 ![]() |
30g Her (6146) | M6-III | 3298 | -4.2 ![]() |
2.0 ![]() |
SW Vir (114961) | M7-III: | 2886 | -4.4 ![]() |
1.3 ![]() |
RX Boo (126327) | M7.5-8 | 2850 | -4.6 ![]() |
1.3 ![]() |
a
Based on the infrared flux method. The
uncertainty in
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