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Query : 2014ApJ...784L..39K |
2014ApJ...784L..39K - Astrophys. J., 784, L39 (2014/April-1)
Intensity enhancement of O VI ultraviolet emission lines in solar spectra due to opacity.
KEENAN F.P., DOYLE J.G., MADJARSKA M.S., ROSE S.J., BOWLER L.A., BRITTON J., McCRINK L. and MATHIOUDAKIS M.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): opacity - radiative transfer - Sun: transition region - Sun: UV radiation
Simbad objects: 4
Number of rows : 4 |
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 | * eps Eri | BY* | 03 32 55.8444911587 | -09 27 29.739493865 | 5.19 | 4.61 | 3.73 | 3.00 | 2.54 | K2V | 1932 | 1 |
2 | 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 |
3 | V* EV Lac | Er* | 22 46 49.7312610268 | +44 20 02.374381562 | 11.85 | 10.26 | 9.89 | M4.0Ve | 902 | 2 | ||
4 | HD 224085 | RS* | 23 55 04.0520383542 | +28 38 01.245426862 | 8.88 | 8.20 | 6.9 | K2+IVeFe-1 | 729 | 0 |
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