Laboratory measurements and astronomical search for cyanomethanimine ⋆

CONTEXT: C-cyanomethanimine (HNCHCN), existing in the two Z and E isomeric forms, is a key prebiotic molecule, but, so far, only the E isomer has been detected toward the massive star-forming region. Sagittarius B2(N) using transitions in the radio wavelength domain. AIMS: With the aim of detecting...

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Publicado en:Astron Astrophys
Autores principales: Melosso, M., Melli, A., Puzzarini, C., Codella, C., Spada, L., Dore, L., Degli Esposti, C., Lefloch, B., Bachiller, R., Ceccarelli, C., Cernicharo, J., Barone, V.
Formato: Artigo
Lenguaje:Inglês
Publicado: 2018
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Article
Acceso en línea:https://ncbi.nlm.nih.gov/pmc/articles/PMC6071866/
https://ncbi.nlm.nih.gov/pubmed/30078846
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1051/0004-6361/201731972
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