discov_num |
notes |
refcode |
CHR 225 |
It in uncertain whether the pair resolved here is the known G8III+A0V |
|
|
composite spectrum binary (Hoffleit & Warren 1991). The small apparent |
Hof1991 |
|
change in theta over the 4-year span between observations does not |
|
|
appear consistent with our estimated period of ~15 or so years; |
|
|
however, the magnitude difference between the components is small, so |
|
|
we are unable to rule out a 180 deg quadrant flip or perhaps an |
|
|
eccentric orbit. |
Hrt1996b |
|
Docobo et al. (2014) use the spectroscopic elements of Carquillat & |
|
|
Prieur (2007), together with speckle data and the Hipparcos parallax, |
Crq2007 |
|
to derive the remaining orbital elements. The resulting masses are |
|
|
1.92 +/- 0.26 and 2.50 +/- 0.29 Msun. |
Doc2014h |
refcode |
metd |
author |
reference |
Doc2014h |
Ma j |
Docobo, J.A. |
................... |
Doc2014h |
|
private communication, 2014 |
|
Doc2014h |
orb j |
Docobo, J.A., Campo, P., Andrade, M., & Horch, E.P. |
2014AstBu..69..461D |
Doc2014h |
|
Astrophys. Bull. 69, 461, 2014 |
|
Hof1991 |
- |
Hoffleit, D. & Jaschek, C. |
1991bsc..book.....H |
Hof1991 |
|
The Bright Star Catalogue, Fifth Revised Edition (preliminary version), 1991 |
|
Hrt1996b |
Sc j |
Hartkopf, W.I., Mason, B.D., McAlister, H.A., Turner, N.H., Barry, D.J., Franz, . |
1996AJ....111..936H |
Hrt1996b |
|
O.G., & Prieto, C.M |
|
Hrt1996b |
|
AJ 111, 936, 1996 |
|