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Forventes på lager: 11-10-2018
Since the discovery of ammonia in the interstellar medium of the Milky Way in 1968, we have identified around 160 complex organic molecules, which help us understand how stars and planets form. IAU S332 describes how such observations, combined with numerical modelling and laboratory astrochemistry, are used to study how the Universe has evolved.
| Forlag | Cambridge University Press |
| Type | Bog |
| Format | Hardback |
| Sprog | Engelsk |
| Udgivelsesdato | 11-10-2018 |
| Første udgivelsesår | 2018 |
| Serie | Proceedings of the International Astronomical Union Symposia and Colloquia |
| Illustrationer | Worked examples or Exercises |
| Fagredaktør | Maria (University of New South Wales Cunningham, Tom (Queen's University Belfast) Millar, Yuri (University of Tokyo) Aikawa |
| Originalsprog | United Kingdom |
| Sideantal | 462 |
| Indbinding | Hardback |
| Forlag | Cambridge University Press |
| Sideoplysninger | 462 pages, Worked examples or Exercises |
| Mål | 181 x 254 x 22 |
| ISBN-13 / EAN-13 | 9781107192577 |