RVs of tidal tails alone cannot yet distinguish between various potentials with flat rotation... or thermal emitters from the hot corona or accretion disk...
Session K1 - Poster Session II.
[K1.027] Magnetohydrodynamic Shock Heating of the Solar Corona... Our technology will distinguish the dominant background of electron recoils caused by...
Sky Observations
The corona is easy to distinguish from the very different halo phenomena, by its smaller size and brighter color. A corona was observed at about 10 pm MST,...
Gamma-Ray Burst Distance Scale
Instead, the observations are consistent with either an extended Galactic halo (often referred to as a corona to distinguish it from the classical Galactic...
SXT Weekly Notes
The solar corona, normally seething with activity but curiously stable on large scales,... images all the time, remarked on the occurrence of a halo CME...
Hot Gaseous Corona of LMC
Coronal C+3 in the Large Magellanic Cloud: Evidence for a Hot Halo 1... s $%5Cmathstrut{^{-1}}$ ), and the interstellar lines are difficult to distinguish...
