CHEMICAL EVOLUTION AND THE GALACTIC HABITABLE ZONE OF M31
We have computed the Galactic Habitable Zones (GHZs) of the Andromeda galaxy (M31) based on the probability of terrestrial planet formation, which depends on the metallicity (Z) of the interstellar medium, and the number of stars formed per unit surface area. The GHZ was obtained from a chemical evo...
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| Gepubliceerd in: | Revista Mexicana de Astronomía y Astrofísica |
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| Hoofdauteurs: | , , |
| Formaat: | Artigo |
| Taal: | Inglês |
| Gepubliceerd in: |
Universidad Nacional Autónoma de México
2013
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| Onderwerpen: | |
| Online toegang: | https://www.redalyc.org/articulo.oa?id=57128966008 |
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