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| Query : 1993AcASn..34..153T |
1993AcASn..34..153T - Acta Astron. Sinica, 34, 153-158 (1993)
HD 105020 probably is a binary with a period of about twenty days.
TAI H.-S., PAN K.-K. and ZHANG Z.-S.
Journal keyword(s):
Simbad objects: 1
| Number of rows : 1 |
| 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 | HD 105020 | V* | 12 05 30.5685391128 | +28 30 20.066603760 | 9.50 | 8.19 | K3III | 27 | 0 |
| Query : 1993AcASn..34..153T |
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HD 105020
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GEN# +1.00105020 |
NSV 5449
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WEB 10500 |
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AG+28 1216
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GSC 01988-00946
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PPM 101630
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YZ 28 5981 |
| AGKR 10837 |
HIC 58971
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SAO 82126
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Gaia DR2 4007075917323087488
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BD+29 2252
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HIP 58971
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TIC 4694122 |
Gaia DR3 4007075917323087488
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| BSD 56-489 | JP11 2156 |
TYC 1988-946-1
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Gaia DR1 4007075913027027072
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| Cl* Melotte 111 AV 60 |
2MASS J12053056+2830200
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UBV M 17711 | |
| GCRV 62960 | NGP 29 41 |
uvby98 100105020
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References (27 between 1850 and 2026) (Total 27)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system). |
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