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Query : 2014ApJ...796L..20S |
2014ApJ...796L..20S - Astrophys. J., 796, L20 (2014/November-3)
Predicting Lyα and Mg II fluxes from K and M dwarfs using galaxy evolution explorer ultraviolet photometry.
SHKOLNIK E.L., ROLPH K.A., PEACOCK S. and BARMAN T.S.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): planet-star interactions - stars: activity - stars: atmospheres - stars: chromospheres
Simbad objects: 28
Number of rows : 28 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | HD 166 | BY* | 00 06 36.7840068588 | +29 01 17.412693890 | 6.82 | 6.07 | 5.6 | G8 | 356 | 0 | ||
2 | V* PW And | RS* | 00 18 20.8895755560 | +30 57 22.129174872 | 9.78 | 8.86 | 8.3 | 7.78 | K2V | 123 | 1 | |
3 | HD 17925 | RS* | 02 52 32.1281856011 | -12 46 10.968056223 | 7.48 | 6.91 | 6.05 | 5.34 | 4.89 | K1V | 514 | 0 |
4 | * eps Eri | BY* | 03 32 55.8444911587 | -09 27 29.739493865 | 5.19 | 4.61 | 3.73 | 3.00 | 2.54 | K2V | 1932 | 1 |
5 | * omi02 Eri | Er* | 04 15 16.3196189945 | -07 39 10.330779018 | 5.69 | 5.25 | 4.43 | 3.74 | 3.29 | K0V | 814 | 0 |
6 | HD 37394 | BY* | 05 41 20.3356800431 | +53 28 51.808818686 | 7.58 | 7.07 | 6.23 | 5.54 | 5.11 | K1 | 329 | 0 |
7 | * chi01 Ori | RS* | 05 54 22.9829893 | +20 16 34.222038 | 5.08 | 5.00 | 4.40 | 3.90 | 3.59 | G0V | 851 | 0 |
8 | HD 43162 | LM* | 06 13 45.2953762392 | -23 51 42.971547996 | 7.068 | 6.366 | 5.94 | 5.61 | G6.5V | 174 | 0 | |
9 | HD 59967 | PM* | 07 30 42.5117581608 | -37 20 21.706958688 | 7.386 | 7.274 | 6.635 | 6.28 | 5.945 | G3V | 162 | 0 |
10 | V* LQ Hya | BY* | 09 32 25.5683895648 | -11 11 04.692242760 | 9.316 | 8.761 | 7.891 | 7.288 | 6.815 | K1Vp | 459 | 0 |
11 | HD 82443 | BY* | 09 32 43.7594578944 | +26 59 18.706023348 | 7.78 | 6.6 | G9V(k) | 248 | 1 | |||
12 | V* AD Leo | Er* | 10 19 36.2808181226 | +19 52 12.010446571 | 10.82 | 9.52 | 9.19 | dM3 | 1340 | 1 | ||
13 | HD 97334 | BY* | 11 12 32.3503039560 | +35 48 50.688978228 | 7.02 | 6.0 | G2 | 283 | 0 | |||
14 | Ross 905 | PM* | 11 42 11.0933350978 | +26 42 23.650782778 | 12.06 | 10.613 | 10.272 | 8.24 | M3V | 645 | 1 | |
15 | HD 106516 | SB* | 12 15 10.55731 | -10 18 44.6354 | 6.44 | 6.57 | 6.11 | F9VFe-1.7CH-0.7 | 421 | 0 | ||
16 | * 61 Vir | PM* | 13 18 24.3139864471 | -18 18 40.297748582 | 5.710 | 5.440 | 4.740 | G6.5V | 674 | 1 | ||
17 | HD 116956 | BY* | 13 25 45.5320130664 | +56 58 13.776984840 | 8.540 | 8.090 | 6.8 | G9V | 126 | 0 | ||
18 | NAME Proxima Centauri | Er* | 14 29 42.9461331854 | -62 40 46.164680672 | 14.21 | 12.95 | 11.13 | 9.45 | 7.41 | M5.5Ve | 1299 | 0 |
19 | V* KU Lib | BY* | 14 40 31.1063299272 | -16 12 33.452598312 | 8.247 | 7.977 | 7.240 | 6.837 | 6.47 | G8Vk: | 98 | 0 |
20 | * ksi Boo A | PM* | 14 51 23.3884659504 | +19 06 01.619801424 | 5.40 | 4.675 | G7Ve | 529 | 0 | |||
21 | HD 197481 | BY* | 20 45 09.5324974119 | -31 20 27.237889841 | 10.05 | 8.627 | 9.078 | 6.593 | M1VeBa1 | 1153 | 0 | |
22 | V* BO Mic | BY* | 20 47 45.0056152368 | -36 35 40.769832192 | 10.39 | 9.337 | 8.216 | K3V(e) | 198 | 0 | ||
23 | HD 203244 | PM* | 21 24 40.5220958049 | -68 13 40.527845137 | 7.70 | 6.97 | G5V | 86 | 0 | |||
24 | HD 204961 | PM* | 21 33 33.9751191976 | -49 00 32.399427028 | 11.359 | 10.176 | 8.672 | 7.665 | 6.479 | M2/3V | 290 | 1 |
25 | HD 209458 | V* | 22 03 10.7727465312 | +18 53 03.549393384 | 8.21 | 7.63 | F9V | 1114 | 1 | |||
26 | * eps Ind | PM* | 22 03 21.6536261624 | -56 47 09.522795714 | 5.75 | 4.69 | K5V | 551 | 0 | |||
27 | BD-15 6290 | BY* | 22 53 16.7325836486 | -14 15 49.304052185 | 12.928 | 11.749 | 10.192 | 9.013 | 7.462 | M3.5V | 1013 | 1 |
28 | HD 220140 | RS* | 23 19 26.6385484104 | +79 00 12.673035540 | 8.43 | 7.54 | 7.17 | 6.76 | G9V | 148 | 1 |
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