WDS 18384+6708 STF 2384 AB : NOTES
| discov_num |
notes |
refcode |
| STF2384 |
Unobserved periastron can be covered by speckle in near future. |
Sod1999 |
|
AB: Malkov et al. (2012) derive dynamical, photometric, and |
|
|
spectroscopic masses 2.03 +/- 0.58, 2.10, and 0.95 Msun, respectively. |
Mlk2012 |
REFERENCES
| refcode |
metd |
author |
reference |
| Hei1996c |
orb - |
Heintz, W.D. |
1996AJ....111..412H |
| Hei1996c |
|
AJ 111, 412, 1996 |
|
| Mlk2012 |
not - |
Malkov, O.Yu., Tamazian, V.S., Docobo, J.A., & Chulkov, D.A. |
2012A&A...546A..69M |
| Mlk2012 |
|
A&A 546, A69, 2012 |
|
| Sod1999 |
orb - |
Soderhjelm, S. |
1999A&A...341..121S |
| Sod1999 |
|
A&A 341, 121, 1999 |
|
DISCOVERER
| idgroup |
discov |
author |
| 1 |
STF |
Struve, F.G.W. |
WDS HISTORIC DATA
| coord_2000 |
discov_num |
comp |
epoch |
obs |
pa |
sep |
mag_pri |
mag_sec |
spectr |
notes |
coord_arcsec_2000 |
| 18384+6708 |
STF2384 |
AB |
2000 |
101 |
131 |
0.2 |
8.31 |
8.95 |
G5 |
NOD |
183823.87+670733.9 |
| 18384+6708 |
STF2384 |
AB |
2020 |
102 |
307 |
0.4 |
8.31 |
8.95 |
G5 |
NO |
183823.66+670735.6 |
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