WDS 00524-6930 DUN 2 (Lam1 Tuc) : NOTES
discov_num |
notes |
refcode |
DUN 2 |
lam 1 Tuc. B is CPD-70@38. |
|
|
SHY 390. Bayesian analysis by Shaya & Olling (2011) indicates very |
Shy2011 |
|
high (near 100%) probability pair is physical. |
|
|
Both A and B are above MS by 2 mag! The parallax can't be wrong. |
Tok2014d |
|
RMK 1. Rectilinear solution by Letchford et al. (2018). |
LRR2018a |
REFERENCES
refcode |
metd |
author |
reference |
LRR2018a |
lin - |
Letchford, R.R., White, G.L. & Ernest, A.D. |
2018JDSO...14..208L |
LRR2018a |
|
JDSO 14, 208, 2018 |
. |
LRR2018b |
orb - |
Letchford, R.R., White, G.L. & Ernest, A.D. |
2018JDSO...14..761L |
LRR2018b |
|
JDSO 14, 761, 2018 |
. |
Shy2011 |
- |
Shaya, E.J. & Olling, R. |
2011ApJS..192....2S |
Shy2011 |
|
ApJS 192, 2, 2011 |
|
Shy2011 |
|
(Statistical analysis of probability that wide Hipparcos pairs are physical. Pairs |
|
Shy2011 |
|
added to WDS only if probability 90% or greater.) |
|
Tok2014d |
E2 - |
Tokovinin, A. |
2014AJ....147...86T |
Tok2014d |
|
AJ 147, 86, 2014 |
|
DISCOVERER
idgroup |
discov |
author |
1 |
DUN |
Dunlop, J. |
WDS HISTORIC DATA
coord_2000 |
discov_num |
comp |
epoch |
obs |
pa |
sep |
mag_pri |
mag_sec |
spectr |
notes |
coord_arcsec_2000 |
00524-6930 |
DUN 2 |
|
1998 |
29 |
81 |
20.4 |
6.70 |
7.35 |
F7IV-V |
N D |
005224.52-693013.6 |
00524-6930 |
DUN 2 |
|
2008 |
31 |
82 |
20.6 |
6.70 |
7.35 |
F7IV-V |
NVD |
005224.52-693013.6 |
00524-6930 |
DUN 2 |
|
2009 |
33 |
82 |
20.4 |
6.70 |
7.35 |
F7IV-V |
NVD |
005224.52-693013.6 |
00524-6930 |
DUN 2 |
|
2013 |
35 |
82 |
20.0 |
6.70 |
7.35 |
F7IV-V |
NVD |
005224.52-693013.6 |
00524-6930 |
DUN 2 |
|
2015 |
37 |
82 |
20.4 |
6.70 |
7.35 |
F7IV-V |
NV |
005224.52-693013.6 |
00524-6930 |
DUN 2 |
|
2021 |
39 |
83 |
20.5 |
6.70 |
7.35 |
F7IV-V |
NV |
005224.52-693013.6 |
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