#1
Posted: Sat Nov 15, 2025 10:31 pm
XRISM’s observations of GX13+1 revealed a slow, fog-like wind instead of the expected high-speed blast, challenging existing models of radiation-driven outflows. The discovery hints that temperature differences in accretion discs may determine how energy shapes the cosmos.
Source: https://www.sciencedaily.com/releases/2 ... 021054.htm
Source: https://www.sciencedaily.com/releases/2 ... 021054.htm