warm-hot intergalactic medium مدیم ِ اندر-کهکشانی ِ گرم-داغ madim-e andar-kahkašâni garm-dâq Fr.: milieu intergalactique chaud The space containing a cluster of galaxies filled with a tenuous gas of
temperature 105 to 107 K and
density 10-6 to 10-4 cm-3. WHIM has been continuously shock-heated during the process of structure formation.
It is so highly ionized that it can only absorb or emit far-ultraviolet and soft X-ray photons, primarily at spectral lines of highly ionized C, O, Ne, and Fe.
WHIM is thought to be the main reservoir of missing baryons. See also: → warm; → hot;
→ intergalactic medium. |