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| Autori principali: | , , , , , , , , , , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2025
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| Soggetti: | |
| Accesso online: | https://arxiv.org/abs/2512.14143 |
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| _version_ | 1866909965176799232 |
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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 |