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Autori principali: Cosentino, Giuliana, Jiménez-Serra, Izaskun, Colzi, Laura, Rivilla, Víctor, Montenegro-Montes, Francisco, Sanz-Novo, Miguel, Rey-Montejo, Marta, Megías, Andrés, Andrés, David San, Martín, Sergio, Zeng, Shaoshan, Godard, Amelie, Requena-Torres, Miguel, Kalvāns, Juris
Natura: Preprint
Pubblicazione: 2025
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Accesso online:https://arxiv.org/abs/2512.14143
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author Cosentino, Giuliana
Jiménez-Serra, Izaskun
Colzi, Laura
Rivilla, Víctor
Montenegro-Montes, Francisco
Sanz-Novo, Miguel
Rey-Montejo, Marta
Megías, Andrés
Andrés, David San
Martín, Sergio
Zeng, Shaoshan
Godard, Amelie
Requena-Torres, Miguel
Kalvāns, Juris
author_facet Cosentino, Giuliana
Jiménez-Serra, Izaskun
Colzi, Laura
Rivilla, Víctor
Montenegro-Montes, Francisco
Sanz-Novo, Miguel
Rey-Montejo, Marta
Megías, Andrés
Andrés, David San
Martín, Sergio
Zeng, Shaoshan
Godard, Amelie
Requena-Torres, Miguel
Kalvāns, Juris
contents There is growing evidence that the Sun might have formed within a nebula impacted by at least one SNR. In this scenario, ejecta and shocks from SNRs may have provided the elements on which life as we know it is based. Investigating the chemical complexity of molecular clouds impacted by SNRs is therefore essential to unveil the star formation process and how life appeared on Earth. In this paper, we exploit this scientific questions and describe which technical specifications will drive in future generation telescopes.
format Preprint
id arxiv_https___arxiv_org_abs_2512_14143
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle The role of supernova remnants for the emergence of pre-biotic chemistry in molecular clouds
Cosentino, Giuliana
Jiménez-Serra, Izaskun
Colzi, Laura
Rivilla, Víctor
Montenegro-Montes, Francisco
Sanz-Novo, Miguel
Rey-Montejo, Marta
Megías, Andrés
Andrés, David San
Martín, Sergio
Zeng, Shaoshan
Godard, Amelie
Requena-Torres, Miguel
Kalvāns, Juris
Astrophysics of Galaxies
There is growing evidence that the Sun might have formed within a nebula impacted by at least one SNR. In this scenario, ejecta and shocks from SNRs may have provided the elements on which life as we know it is based. Investigating the chemical complexity of molecular clouds impacted by SNRs is therefore essential to unveil the star formation process and how life appeared on Earth. In this paper, we exploit this scientific questions and describe which technical specifications will drive in future generation telescopes.
title The role of supernova remnants for the emergence of pre-biotic chemistry in molecular clouds
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2512.14143