WDS 23317+1956 WIR 1 AB (EQ Peg) : NOTES
| discov_num |
notes |
refcode |
| WIR 1 |
This is the flare star EQ Peg. Component B is suspected to be the |
|
|
source of the flares, although both components may be flare stars. |
|
|
See Baize & Petit (1989) catalog of doubles with variable component. |
Baz1989d |
|
AB: Additional notes may be found in Wilson (1954). |
WRH1954a |
| LMP 24 |
AC: Rectilinear solution by Mason & Hartkopf (2016). |
Msn2016a |
REFERENCES
| refcode |
metd |
author |
reference |
| Baz1989d |
- |
Baize, P. & Petit, M. |
1989A&AS...77..497B |
| Baz1989d |
|
A&AS 77, 497, 1989 |
|
| Kpp2020f |
Hg+ j |
Knapp, W.R.A. |
2020JDSO...16..229K |
| Kpp2020f |
+C |
JDSO 16, 229, 2020 |
|
| Kpp2020f |
+orb
|
|
|
| Msn2016a |
lin - |
Mason, B.D. & Hartkopf, W.I. |
2016IAUDS.189....1M |
| Msn2016a |
|
Inf. Circ. 189, 1, 2016 |
|
| WRH1954a |
J j |
Wilson, R.H. |
1954AJ.....59..132W |
| WRH1954a |
+Ma |
AJ 59, 132, 1954 |
|
DISCOVERER
| idgroup |
discov |
author |
| 1 |
LMP |
Lampens, P. & Strigachev, A. |
| 21 |
WIR |
Wirtanen, C.A. |
WDS HISTORIC DATA
| coord_2000 |
discov_num |
comp |
epoch |
obs |
pa |
sep |
mag_pri |
mag_sec |
spectr |
notes |
coord_arcsec_2000 |
| 23317+1956 |
WIR 1 |
AB |
2007 |
51 |
86 |
5.4 |
10.52 |
12.40 |
M4+M5 |
NO V |
233151.83+195614.7 |
| 23317+1956 |
WIR 1 |
AB |
2010 |
53 |
82 |
5.3 |
10.52 |
12.40 |
M4+M5 |
NO |
233152.17+195614.2 |
| 23317+1956 |
WIR 1 |
AB |
2011 |
58 |
82 |
5.4 |
10.52 |
12.40 |
M4 M5 |
NO |
233152.17+195614.2 |
| 23317+1956 |
WIR 1 |
AB |
2012 |
61 |
80 |
5.5 |
10.52 |
12.40 |
M3.5V+M5V |
NO |
233152.17+195614.2 |
| 23317+1956 |
WIR 1 |
AB |
2013 |
65 |
79 |
5.1 |
10.52 |
12.40 |
M3.5V+M5V |
NO |
233152.24+195614.0 |
| 23317+1956 |
WIR 1 |
AB |
2015 |
68 |
78 |
5.4 |
10.52 |
12.40 |
M3.5V+M5V |
NO |
233152.24+195614.0 |
| 23317+1956 |
WIR 1 |
AB |
2017 |
72 |
76 |
5.4 |
10.52 |
12.40 |
M3.5V+M5V |
NO |
233152.24+195614.0 |
| 23317+1956 |
WIR 1 |
AB |
2020 |
73 |
73 |
5.3 |
10.52 |
12.40 |
M3.5V+M5V |
NO |
233152.24+195614.0 |
If you need more information about this double, apply for a
data request form to the WDS.
