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.
from All Top News -- ScienceDaily https://ift.tt/icQKarB
from All Top News -- ScienceDaily https://ift.tt/icQKarB
Comments
Post a Comment