Portal de Periódicos da CAPES

Seeds of Life in Space (SOLIS)

2017; EDP Sciences; Volume: 605; Linguagem: Inglês

10.1051/0004-6361/201731249

1432-0746

C. Codella, C. Ceccarelli, P. Caselli, Nadia Balucani, Vincenzo Barone, F. Fontani, B. Leflóch, L. Podio, S. Viti, Siyi Feng, R. Bachiller, E. Bianchi, F. Dulieu, I. Jiménez-Serra, Jonathan Holdship, R. Neri, J. E. Pineda, Andy Pon, Ian Sims, S. Spezzano, A. I. Vasyunin, F. O. Alves, L. Bizzocchi, S. Bottinelli, E. Caux, A. Chacón-Tanarro, R. Choudhury, A. Coutens, Cécile Favre, P. Hily-Blant, C. Kahane, A. Jaber Al-Edhari, J. Laas, A. López-Sepulcre, J. Ospina, Yoko Oya, A. Punanova, Cristina Puzzarini, D. Quénard, Albert Rimola, Nami Sakai, Dimitrios Skouteris, V. Taquet, L. Testi, P. Theulé, Piero Ugliengo, C. Vastel, Fanny Vazart, L. Wiesenfeld, Satoshi Yamamoto,

Astro and Planetary Science

Context. Modern versions of the Miller-Urey experiment claim that formamide (NH2CHO) could be the starting point for the formation of metabolic and genetic macromolecules. Intriguingly, formamide is indeed observed in regions forming solar-type stars and in external galaxies.