On the verge of a possible
Here is the Wolf Rye star system
WR 111 (FNG 3).
The star is located in a congregation of magnetars
SGR 1860-20.
Star
100% doubleBut perhaps there are other companions in this system
![Думаю :think:](./images/smilies/smile_think.gif)
.
I've decided to do some scientific work and found out that the spectrum and computer moderation suggest that a star with parameters almost similar to Sirius A (probable mass
2 MSol) and a dim orange dwarf with mass
0.525 MSol may be located in more distant orbits.
If so, the eccentricity of hypothetical
WR 111d C should be 0.3.
Orange dwarf
WR 111d D has almost zero eccentricity
My hypothesis of the multiplicity of the WR 111 system cannot be tested at this time.
The system is on a different side of the galaxy, the research is hampered by interstellar dust and other smaller scattered clusters and their molecular clouds.
So these objects are labeled as hypothetical
I guess we won't be able to check the system soon.
That's too bad.
I wanted to open my multiple star system.