WDS 15529+1526 MUG 21 Ba,Bb : NOTES
| discov_num |
notes |
refcode |
| MUG 21 |
Mugrauer & Ginski (2015) note that the B component is itself a close |
|
|
binary, with projected separation about 4.3 +/- 0.7 au. The orbital |
|
|
period is estimated as 8.5 +/- 2 yr, assuming a total system mass of |
|
|
1.12 Msun. |
Mug2015 |
REFERENCES
| refcode |
metd |
author |
reference |
| Mug2015 |
A j |
Mugrauer, M. & Ginski, C. |
2015MNRAS.450.3127M |
| Mug2015 |
|
MNRAS 450, 3127, 2015 |
|
WDS HISTORIC DATA
| coord_2000 |
discov_num |
comp |
epoch |
obs |
pa |
sep |
mag_pri |
mag_sec |
spectr |
notes |
coord_arcsec_2000 |
| 15529+1526 |
MUG 21 |
Ba,Bb |
2017 |
3 |
86 |
0.1 |
10.50 |
10.50 |
|
N K |
155256.28+152550.5 |
| 15529+1526 |
MUG 21 |
Ba,Bb |
2018 |
4 |
111 |
0.1 |
10.50 |
10.50 |
|
N K |
155256.28+152550.5 |
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