Acircumstellar envelope (CSE) is a part of a star that has a roughly spherical shape and is not gravitationally bound to the star core. Usually circumstellar envelopes are formed from the dense stellar wind, or they are present before the formation of the star.[1] Circumstellar envelopes of old stars (Mira variables and OH/IR stars) eventually evolve into protoplanetary nebulae, and circumstellar envelopes of young stellar objects evolve into circumstellar discs.[2]
|
| |||||||
|---|---|---|---|---|---|---|---|
| |||||||
| Formation |
| ||||||
| Evolution |
| ||||||
| Classification |
| ||||||
| Nucleosynthesis |
| ||||||
| Structure |
| ||||||
| Properties |
| ||||||
| Star systems |
| ||||||
| Earth-centric observations |
| ||||||
| Lists |
| ||||||
| Related |
| ||||||
| |||||||
 | This article about stellar evolution is a stub. You can help Wikipedia by expanding it. |
