discov_num |
notes |
refcode |
TOK 414 |
HIP 83962 = HR 6375 has a variable RV according to the GCS, while |
|
|
Gorynya (2013, private communication) detected double lines. It is |
|
|
resolved tentatively at 33mas with dy=1.8 mag (the 5-ms exposure makes |
|
|
it unlikely that the asymmetry is caused by vibrations). The |
|
|
separation corresponds to an orbital period on the order of 1yr, which |
|
|
could bias the Hipparcos parallax. However, Eggleton & Tokovinin |
|
|
(2008 MNRAS 389, 869) consider the star as single. The new pair was |
|
|
not resolved in 2014.3, presumably it became closer. |
Tok2015c |