IRS 16SW
Massive stellar system within the S-cluster at the galactic-center, located in immediate proximity to the supermassive black hole sagittarius-a. Part of the IRS 16 complex; IRS 16SW denotes the southwest component.
Characteristics
- Modeled as a high-mass binary or triple system comprising evolved massive stars, potentially Wolf-Rayet types or O-type stars.
- Subject to extreme tidal forces due to proximity to sagittarius-a.
Recent Findings
- G-objects near sagittarius-a resolved as stellar debris/clouds originating from interactions with IRS 16SW binary stars.
- Analysis confirms G-objects are products of IRS 16SW binary evolution or disruption events.
- See full integration: Resolved: G-Objects Near SgrA* Originate from IRS 16SW Binary Stars