Non-radial oscillations in the giant star xi Hya

A computer-generated illustration of one possible non-radial oscillation mode in the giant star xi Hya. The blue parts contain particles in the upper stellar atmosphere moving away from the stellar centre, hence they cause a "blue-shift" (towards shorter wavelengths) in the spectrum for the observer. At the same time, particles in the red parts move towards the stellar centre and cause a "red-shift" (towards longer wavelengths). Particles in the white regions do not move during the oscillation cycle. Half an oscillation cycle later, the red parts will have become blue and vice versa.

Të drejtat:
ESO

Rreth fotografisë

Id:eso0215b
Tipi:Simulim
Data e Publikimit:15 Maj 2002
Publikime të ngjashme:eso0215
Përmasat:785 x 778 px

Rreth objektit

Emri:xi Hya
Tipi:Milky Way : Star : Evolutionary Stage : Red Giant
Distanca:130 vite dritë
Kategori:Stars

Formate Fotografish

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