CPD−64 2731: a massive spun-up and rejuvenated high-velocity runaway star
2021
Konferenz
Zugriff:
During our search for massive stars on late evolutionary stages in the WISE archive we discovered a high-velocity runaway star CPD-64o 2731, associated with a horseshoe-shaped nebula. Its spectral type is O5.5Vn((f)) and projected rotational velocity is ≈ 300 km/s, which is extremely high for this spectral type. The kinematic age of ≈ 6 Myr, assuming it was born near the Galactic plane, exceeds its age derived from single star models by a factor of two. These properties suggest that CPD-64o 2731 is a rejuvenated and spun-up binary product. The geometry of the nebula and the almost central location of the star within it argue against a pure bow shock interpretation for it. Instead, we suggest that the binary interaction happened recently, thereby creating the nebula, with a cavity blown by the current fast stellar wind. This conclusion is supported by our results of 2D numerical hydrodynamic modeling.
Titel: |
CPD−64 2731: a massive spun-up and rejuvenated high-velocity runaway star
|
---|---|
Autor/in / Beteiligte Person: | Maryeva, Olga ; Gvaramadze, Vasilii ; Kniazev, Alexei ; Alexashov, Dmitry ; Castro, Norberto ; Langer, Norbert ; Katkov, Ivan |
Link: | |
Veröffentlichung: | 2021 |
Medientyp: | Konferenz |
DOI: | 10.5281/zenodo.5535106 |
Schlagwort: |
|
Sonstiges: |
|