WDS 23317+1956 LMP 24 AC : 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 |
|
| 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 |
LMP 24 |
AC |
1953 |
1 |
60 |
49.0 |
10.52 |
11.50 |
M4 |
|
233151.83+195614.7 |
| 23317+1956 |
LMP 24 |
AC |
1997 |
3 |
35 |
34.0 |
10.52 |
12.23 |
M4 |
D |
233152.17+195614.2 |
| 23317+1956 |
LMP 24 |
AC |
2010 |
4 |
23 |
30.8 |
10.52 |
12.23 |
M4 |
N D |
233152.17+195614.2 |
| 23317+1956 |
LMP 24 |
AC |
2011 |
8 |
22 |
31.3 |
10.52 |
12.23 |
M4 |
N D |
233152.17+195614.2 |
| 23317+1956 |
LMP 24 |
AC |
2012 |
10 |
22 |
30.7 |
10.52 |
12.23 |
M4 |
N |
233152.17+195614.2 |
| 23317+1956 |
LMP 24 |
AC |
2013 |
12 |
20 |
31.0 |
10.52 |
12.33 |
M3.5V |
N |
233152.24+195614.0 |
| 23317+1956 |
LMP 24 |
AC |
2015 |
13 |
18 |
30.7 |
10.52 |
12.33 |
M3.5V |
NL |
233152.24+195614.0 |
| 23317+1956 |
LMP 24 |
AC |
2017 |
14 |
16 |
30.4 |
10.52 |
12.33 |
M3.5V |
NL |
233152.24+195614.0 |
| 23317+1956 |
LMP 24 |
AC |
2020 |
15 |
13 |
30.2 |
10.52 |
12.33 |
M3.5V |
NL |
233152.24+195614.0 |
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