WDS 00152+2722 J 868 : NOTES
| discov_num |
notes |
refcode |
| J 868 |
Rectilinear solution by Rica (2014). |
FMR2014f |
|
Due to the very different parallax in Gaia DR2 for the two components |
Cve2019b |
|
the orbital solution of Novakovic (2007) is no longer plausible and the |
Nov2007b |
|
linear solution is preferred. The orbit solution is retained in ORB6. |
|
| J 868 |
Despite having an orbit, this pair determined to be optical. |
FMR2014d |
REFERENCES
| refcode |
metd |
author |
reference |
| Cve2019b |
C |
Cvetkovic, Z., Pavlovic, R. & Boeva, S. |
2019AJ....158..215C |
| Cve2019b |
|
AJ 158, 215, 2019 |
|
| FMR2014d |
not - |
Rica Romero, F.M. |
................... |
| FMR2014d |
|
Webb Soc., Double Star Circ. 22, 2014 |
|
| FMR2014f |
orb - |
Rica Romero, F.M. |
2014IAUDS.184....1R |
| FMR2014f |
+lin |
Inf. Circ. 184, 1, 2014 |
|
| Nov2007a |
orb - |
Novakovic, B. |
2007IAUDS.162....1N |
| Nov2007a |
|
Inf. Circ. 162, 1, 2007 |
|
| Nov2007b |
orb - |
Novakovic, B. |
2007BaltA..16..435B |
| Nov2007b |
|
Baltic Astron. 16, 435, 2007 |
|
DISCOVERER
| idgroup |
discov |
author |
| 1 |
J |
Jonckheere, R. |
WDS HISTORIC DATA
| coord_2000 |
discov_num |
comp |
epoch |
obs |
pa |
sep |
mag_pri |
mag_sec |
spectr |
notes |
coord_arcsec_2000 |
| 00152+2722 |
J 868 |
|
2006 |
19 |
230 |
5.8 |
12.42 |
12.62 |
|
ODB |
001509.80+272345.1 |
| 00152+2722 |
J 868 |
|
2011 |
23 |
230 |
6.0 |
12.42 |
12.62 |
|
ODB |
001509.80+272345.1 |
| 00152+2722 |
J 868 |
|
2013 |
25 |
231 |
6.0 |
12.42 |
12.62 |
F4V+G5V |
NOUB |
001509.80+272345.1 |
| 00152+2722 |
J 868 |
|
2015 |
29 |
231 |
6.2 |
12.42 |
12.62 |
F4V+G5V |
NOUB |
001509.94+272346.7 |
| 00152+2722 |
J 868 |
|
2016 |
30 |
231 |
6.2 |
12.42 |
12.62 |
F4V+G5V |
NO B |
001509.94+272346.7 |
| 00152+2722 |
J 868 |
|
2018 |
36 |
232 |
6.3 |
12.42 |
12.62 |
F4V+G5V |
NL B |
001509.94+272346.7 |
| 00152+2722 |
J 868 |
|
2020 |
38 |
232 |
6.4 |
12.42 |
12.62 |
F4V+G5V |
NL B |
001509.94+272346.7 |
If you need more information about this double, apply for a
data request form to the WDS.
