Two newly identified eclipsing binaries in open cluster NGC 3532

@inproceedings{Ozdarcan2021TwoNI,
  title={Two newly identified eclipsing binaries in open cluster NGC 3532},
  author={Orkun Ozdarcan},
  year={2021}
}
We present light curve analyses of two newly identified detached eclipsing binaries, HD96609 and HD303734, in the region of the richly populated open cluster NGC3532. HD96609 is composed of two main sequence stars (B9-A0V + A2V) with masses and radii of M1 = 2.66 ± 0.02M , M2 = 1.84 ± 0.01M , R1 = 2.740 ± 0.006R , R2 = 1.697 ± 0.005R . The positions of the components on log M − log R plane suggests log(age/yr) 8.55, corresponding 350 ± 40 Myr of age, which agrees with the 300 ± 100 Myr age of… 

Figures and Tables from this paper

References

SHOWING 1-3 OF 3 REFERENCES
Lightkurve: Kepler and TESS
  • Computing in Science & Engineering,
  • 2007
The Observation and Analysis of Stellar Photospheres, 3 edn
  • 2005