nep |
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Spectral type | notes |
*20 | -17.3 ![]() |
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<4.3 | 5310 ![]() |
<0.68 | <0.77 | G8 | |
260 | -19.5 ![]() |
11.1 ![]() |
112.4 | 5790 ![]() |
2.76 ![]() |
2.71 ![]() |
G2 | |
330 | -35.4 ![]() |
6.7 ![]() |
<3.6 | 5250 ![]() |
<0.53 | G9 | ||
370 | -15.7 ![]() |
7.0 ![]() |
119.3 | 6250 ![]() |
3.22 ![]() |
3.09 ![]() |
F8 | |
*1420 | 22.7 ![]() |
- | 5150 ![]() |
K0 | ||||
*1441 | -15.7 ![]() |
4.0 ![]() |
56.2 | 5790 ![]() |
2.34 ![]() |
2.34 ![]() |
G2 | |
1470 | -10.2 ![]() |
7.4 ![]() |
106.2 | 5310 ![]() |
2.22 ![]() |
2.27 ![]() |
G8 | |
1500 | -17.0 ![]() |
5.5 ![]() |
10.7 | 5790 ![]() |
1.57 ![]() |
1.59 ![]() |
G2 | |
1511 | 87.0 | 4450 ![]() |
1.01 ![]() |
K4 (?) | x | |||
1580 | 65.1 | 4830 ![]() |
1.36 ![]() |
1.55 ![]() |
K2 (?) | x | ||
*1600 | -18.8 ![]() |
5.4 ![]() |
- | 5790 ![]() |
G2 | |||
1601 | -13.0 ![]() |
11.0 ![]() |
135.6 | 5940 ![]() |
3.05 ![]() |
2.94 ![]() |
G0 | |
1690 | -37.0 ![]() |
10.1 ![]() |
- | 5790 ![]() |
G2 | |||
1800 | -58.0 ![]() |
16.3 ![]() |
98.1 | 6650 ![]() |
3.28 ![]() |
3.16 ![]() |
F5 | |
1840 | ![]() |
- | 5940 ![]() |
G0 | ||||
1960 | ![]() |
- | 7000 ![]() |
F2 | ||||
2050 | -7.6 ![]() |
12.8 ![]() |
77.2 | 5150 ![]() |
1.85 ![]() |
1.96 ![]() |
K0 | |
2100 | - | 3500 ![]() |
M3 | |||||
2210 | -7.1 ![]() |
25.0 ![]() |
- | 6250 ![]() |
F8 (?) | x | ||
2250 | -7.4 ![]() |
3.8 ![]() |
<3.0 | 5150 ![]() |
<0.33 | K0 | ||
2360 | -26.2 ![]() |
8.2 ![]() |
44.9 | 6250 ![]() |
2.63 ![]() |
2.58 ![]() |
F8 | |
2400 | -14.3 ![]() |
4.5 ![]() |
<3.9 | 5790 ![]() |
<1.12 | <1.16 | G2 | |
2470 | 8.3 ![]() |
- | 6950 ![]() |
F3 | ||||
2480 | ![]() |
- | 5150 ![]() |
K0 | ||||
*2970 | ![]() |
- | 7000 ![]() |
F2 (?) | x | |||
*3080 | -12.9 ![]() |
20.6 ![]() |
147.6 | 4800 ![]() |
1.85 ![]() |
2.00 ![]() |
K2.5 (?) | x |
3220 | -25.1 ![]() |
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<5.4 | 5150 ![]() |
<0.60 | <0.72 | K0 | |
3560 | -2.6 ![]() |
7.9 ![]() |
124.9 | 5310 ![]() |
2.34 ![]() |
2.38 ![]() |
G8 | |
3610 | +9.7 ![]() |
5.1 ![]() |
13.9 | 4450 ![]() |
0.11 ![]() |
K4 | ||
3690 | - | 9000 ![]() |
A2 | |||||
3710 | ![]() |
- | 7000 ![]() |
F2 | ||||
*4090 | -40.7 ![]() |
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- | 5790 ![]() |
G2 | |||
4100 | +10.0 ![]() |
4.5 ![]() |
18.2 | 5150 ![]() |
1.14 ![]() |
1.27 ![]() |
K0 | |
4130 | ![]() |
- | 6650 ![]() |
F5 | ||||
4180 | -13.6 ![]() |
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<3.0 | 5150 ![]() |
<0.33 | K0 | ||
4380 | -21.8 ![]() |
6.3 ![]() |
29.0 | 5560 ![]() |
1.81 ![]() |
1.86 ![]() |
G5 | |
4470 | -13.5 ![]() |
5.3 ![]() |
24.3 | 4800 ![]() |
0.85 ![]() |
1.06 ![]() |
K3 | |
4530 | -21.6 ![]() |
14.2 ![]() |
228.7 | 5300 ![]() |
2.97 ![]() |
2.84 ![]() |
G9 | |
4780 | -26.3 ![]() |
11.7 ![]() |
422.3 | 4830 ![]() |
3.60 ![]() |
3.40 ![]() |
K2 | |
4810 | -37.0 ![]() |
7.8 ![]() |
- | 6650 ![]() |
F5 | |||
*4931 | +2.5 ![]() |
3.6 ![]() |
<5.5 | 4000 ![]() |
<-0.8 | K8 | ||
4970 | +14.3 ![]() |
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<8.6 | 4830 ![]() |
<0.41 | K2 | ||
5060 | -2.3 ![]() |
7.6 ![]() |
97.9 | 5560 ![]() |
2.44 ![]() |
2.45 ![]() |
G5 | |
5220 | -18.9 ![]() |
25.8 ![]() |
<4.8 | 6250 ![]() |
<1.61 | <1.59 | F8 | |
*5320 | -19.4 ![]() |
4.0 ![]() |
38.5 | 5150 ![]() |
1.49 ![]() |
1.62 ![]() |
K0 | |
5510 | -53.5 ![]() |
20.4 ![]() |
371.3 | 5150 ![]() |
3.79 ![]() |
3.46 ![]() |
K0 (?) | x |
5520a | +8.0 ![]() |
7.6 ![]() |
93.2 | 4450 ![]() |
1.05 ![]() |
K4 (?) | SB2 | |
5520b | +25.7 ![]() |
4.2 ![]() |
39.8 | 4450 ![]() |
0.60 ![]() |
K4 (?) | ||
5950 | -20.6 ![]() |
11.4 ![]() |
<4.3 | 5940 ![]() |
<1.30 | <1.31 | G0 | |
6030 | -13.2 ![]() |
4.5 ![]() |
<5.0 | 4780 ![]() |
<0.11 | K3 | ||
6051 | -9.1 ![]() |
15.1 ![]() |
- | 4410 ![]() |
K5 | |||
6160 | - | 7300 ![]() |
F0 | |||||
6163 | -7.4 ![]() |
3.7 ![]() |
49.4 | 5700 ![]() |
2.19 ![]() |
2.21 ![]() |
G3 | |
6350 | ![]() |
- | 3500 ![]() |
M3 | ||||
6400 | -23.9 ![]() |
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<5.0 | 4830 ![]() |
<0.17 | K2 | ||
6410 | -25.6 ![]() |
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10.5 | 5150 ![]() |
0.89 ![]() |
1.02 ![]() |
K0 | |
6510 | - | 7300 ![]() |
F0 |
Note: an x in column eight indicates that the star is (or it is supposed to be) binary. We indicate SB2 for double-lined spectroscopic
binary. * We lack the thorium-argon lamp exposures for the nights in which these stars were acquired. They were wavelength calibrated using lamp exposures of the nearest night. a Primary and b secondary component of nep 5520 SB2 system. |