X-ray emission characteristics of an O+O binary HD 93205
Abstract
A detailed X-ray study of a massive binary called HD 93205 has been made using long-term XMM-Newton observations. The X-ray spectrum of HD 93205 displays negligible counts above 5 keV. The two thermal plasma emission models with average temperature values as ∼ 0.20 and ∼ 0.60 keV are required to explain the X-ray spectra. The X-ray flux variations in the binary are noticed to be in qualitative agreement with the wind-wind collision model but with a few deviations from the expected 1/D trend (D is the binary separation).
- Publication:
-
IAU Symposium
- Pub Date:
- 2024
- DOI:
- 10.1017/S1743921322002721
- Bibcode:
- 2024IAUS..361..323A
- Keywords:
-
- Stars:early-type;
- binaries:colliding-winds;
- X-rays:stars;
- stars:individual: HD 93205