| discov_num |
notes |
refcode |
| STI2051 |
A is an astrometric binary. B (mag. 12.44, 8", DC) is a white dwarf, |
|
|
in slow retrograde motion about the mass-center. A very large proper |
|
|
proper motion brought this pair close to a 13th magnitude star which |
|
|
was measured as the C component by Pauwels & Lampens. |
Pws1993 |
|
Also known as HDS 584. |
|
|
B: Teff = 7122 +/- 122 K, R = 0.0114 +/- 0.0004 \rsun, M = 0.675 +/- |
BdH2017b |
|
0.051 \msun. |
|
|
AB: Rectilinear solutions by Cvetkovic (2015) |
Cve2015b |
|
and Cvetkovic et al. (2016). |
Cve2016 |
|
Despite the linear solution, based on proper motion and parallax |
|
|
is physical. |
|
| refcode |
metd |
author |
reference |
| BdH2017b |
not - |
Bond, H.E., Bergeron, P. & Bedard, A. |
2017ApJ...848...16B |
| BdH2017b |
|
ApJ 848, 16, 2017 |
|
| Cve2015b |
orb - |
Cvetkovic, Z. |
2015IAUDS.187....1C |
| Cve2015b |
+lin |
Inf. Circ. 187, 1, 2015 |
|
| Cve2016 |
C j |
Cvetkovic, Z., Pavlovic, R. & Boeva, S. |
2016AJ....151...58C |
| Cve2016 |
+lin |
AJ 151, 58, 2016 |
|
| Kpp2020f |
Hg+ j |
Knapp, W.R.A. |
2020JDSO...16..229K |
| Kpp2020f |
+C |
JDSO 16, 229, 2020 |
|
| Kpp2020f |
+orb
|
|
|
| Pws1993 |
Pa - |
Pauwels, T. & Lampens, P. |
1993BAORB..10..216P |
| Pws1993 |
|
Bull. R. Astron. Obs. Belgium 10, 216, 1993 |
|
