Physics and chemistry of gas in planetary nebulaeBernard Salas, J., 2003, Groningen: s.n.. 183 p.
Research output: Thesis › Thesis fully internal (DIV) › Academic
Stars are born, live and die similarly to any human being in the Universe. This thesis deals with the final stages of evolution (life) experíenced by stars like our Sun prior to their death, the so-called Planetary Nebula phase. In 5 billion years our Sun also will experience this phase and will become a Planetary Nebula: a shell of gas, which is the remnant of what was once the envelope of the star. This material slowly coasts away from the star and will eventually merge with other material in space. ... Zie: Summary
|Qualification||Doctor of Philosophy|
|Place of Publication||Groningen|
|Publication status||Published - 2003|
- Proefschriften (vorm), Gassen, Interplanetaire materie, Planetaire nevels, Astrochemie, Astrofysica, 39.22
No data available