Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8141377 | New Astronomy | 2018 | 6 Pages |
Abstract
The mass of the primary and secondary stars are calculated to be M1 = 1.18Mâ(â¯Â±â¯0.08) and M2 = 0.21Mâ(â¯Â±â¯0.01) indicating the primary to be underluminous for its mass and the secondary to be overluminous for its mass.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
M. Martignoni, C. Barani, F. Acerbi,