discov_num |
notes |
refcode |
A 2413 |
Component variable? |
Hln1963 |
|
See Baize & Petit (1989) catalog of doubles with variable component. |
Baz1989d |
|
According to Scardia et al. (2001), this orbit is now well defined and |
Sca2001d |
|
will certainly change little in the future; only the period is still |
|
|
slightly uncertain. The Hipparcos parallax is 0".02012 +/- 0.00150. |
|
|
This gives a mass sum of 2.1 Msun +/- 29%, agreeing very well with |
|
|
expected values for a system of type G0. Compared to the orbit |
|
|
calculated by Scardia in 1980, the total mass of the system, whose |
Sca1980e |
|
uncertainty was then 55%, is now much better defined. The dynamical |
|
|
parallax is 0".0193, well in agreement with the measured parallax. |
|
|
Malkov et al. (2012) derive dynamical, photometric, and spectroscopic |
|
|
masses of 1.64 +/- 0.52, 2.04, and 1.05 Msun, respectively. |
Mlk2012 |
refcode |
metd |
author |
reference |
Baz1989d |
- |
Baize, P. & Petit, M. |
1989A&AS...77..497B |
Baz1989d |
|
A&AS 77, 497, 1989 |
|
Hln1963 |
Ma j |
Holden, F. |
1963JO.....46..131H |
Hln1963 |
|
J. Obs. 46, 131, 1963 |
|
Mlk2012 |
not - |
Malkov, O.Yu., Tamazian, V.S., Docobo, J.A., & Chulkov, D.A. |
2012A&A...546A..69M |
Mlk2012 |
|
A&A 546, A69, 2012 |
|
Msn2021c |
orb - |
Josties, J. & Mason, B.D. |
2021IAUDS.205....1M |
Msn2021c |
|
Inf. Circ. 205, 1, 2021 |
|
Sca1980e |
orb - |
Scardia, M. |
1980AN....301..241S |
Sca1980e |
|
AN 301, 241, 1980 |
|
Sca2001d |
orb - |
Scardia, M., Prieur, J.-L., Koechlin, L., & Aristidi, E. |
2001AN....322..161S |
Sca2001d |
|
AN 322, 161, 2001 |
|