2 papers
astro-ph.SR2025
Differentiating the acceleration mechanisms in the slow and Alfvénic slow solar wind
Yeimy J. Rivera, Samuel T. Badman, J. L. Verniero +18
In the corona, plasma is accelerated to hundreds of kilometers per second, and heated to temperatures hundreds of times hotter than the Sun's surface, before it escapes to form the…
astro-ph.HE2016
An Ultra-Fast X-ray Disk Wind in the Neutron Star Binary GX 340+0
J. M. Miller, J. Raymond, E. Cackett +2
We present a spectral analysis of a brief Chandra/HETG observation of the neutron star low-mass X-ray binary GX~340+0. The high-resolution spectrum reveals evidence of ionized abso…