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Birth, Evolution and Death of Stars


Engels | 22-08-2013 | 172 pagina's

9789814508773

Paperback / softback


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Tekst achterflap

It has been known for a long time that stars are similar to our Sun. But it was only in 1810 that they were shown to be made of an incandescent gas. The chemical composition of this gas began to be determined in 1860. In 1940, it was demonstrated that the energy radiated by the stars is of thermonuclear origin. How stars form from interstellar matter and how they evolve and die was understood only recently, with our knowledge still incomplete. It was also realized recently that close double stars present a wide variety of extraordinary phenomena, which are far from being completely explored.

Details

EAN :9789814508773
Auteur: 
Uitgever :World Scientific Publishing Company
Publicatie datum :  22-08-2013
Uitvoering :Paperback / softback
Taal :Engels
Hoogte :229 mm
Breedte :152 mm
Dikte :10 mm
Gewicht :259 gr
Status :POD (Beschikbaar als print-on-demand.)
Aantal pagina's :172