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| Query : 1989AcApS...9..201L |
1989AcApS...9..201L - Acta Astrophys. Sinica, 9, 201 (1989)
A possible mechanism for the microwave radiation from the quiescent coronae of late-type stars.
LI H.W.
Journal keyword(s):
Simbad objects: 5
| Number of rows : 5 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | G 272-61B | PM* | 01 39 01.6377185550 | -17 57 01.001240728 | M6V | 892 | 0 | |||||
| 2 | V* YY Gem | SB* | 07 34 37.4474327544 | +31 52 10.179641496 | 11.60 | 10.56 | 9.27 | 7.69 | 6.67 | M0.5VeFe-2 | 882 | 0 |
| 3 | HD 152751 | ** | 16 55 28.7575690 | -08 20 10.787849 | 11.647 | 10.593 | 9.023 | 7.937 | 6.565 | M3.5Ve | 547 | 1 |
| 4 | HD 197481 | BY* | 20 45 09.5324974119 | -31 20 27.237889841 | 10.05 | 8.627 | 9.078 | 6.593 | M1VeBa1 | 1344 | 0 | |
| 5 | BD+19 5116 | ** | 23 31 52.17898 | +19 56 14.1505 | 12.737 | 11.749 | 10.165 | 8.982 | 7.446 | M3.5V | 469 | 0 |
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