Revealing the baryon cycle in Galaxy Clusters: connecting galaxy dynamics and gas thermodynamics using (sub-)mm-wave and optical IFU surveys
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arXiv
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| Autores principales: | , , , , , , , , , , |
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| Formato: | Preprint |
| Publicado: |
2025
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| _version_ | 1866909965294239744 |
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| author | Montenegro-Montes, Francisco M. Sánchez-Blázquez, Patricia Mroczkowski, Tony de Paz, Armando Gil Catalán-Torrecilla, Cristina Gendron-Marsolais, Marie-Lou Macías-Pardo, Paula Callejas-Córdoba, Beatriz Montaña, Alfredo Macías-Pérez, Juan F. Planelles, Susana |
| author_facet | Montenegro-Montes, Francisco M. Sánchez-Blázquez, Patricia Mroczkowski, Tony de Paz, Armando Gil Catalán-Torrecilla, Cristina Gendron-Marsolais, Marie-Lou Macías-Pardo, Paula Callejas-Córdoba, Beatriz Montaña, Alfredo Macías-Pérez, Juan F. Planelles, Susana |
| contents | Observations in the visible and near infrared are transforming our view of the processes affecting galaxy evolution, much of which is dominated by interactions with the large scale environment. Yet a complete picture is missing, as no corresponding high resolution view of the warm/hot intracluster, circumgalactic, and intergalactic media exists over large areas and a comparably broad range of redshifts. Combined with wide-field optical IFU surveys such as CATARSIS, a large diameter sub-mm telescope with a degree-scale field of view would enable a joint view of galaxy dynamics and gas thermodynamics, transforming our understanding of environmental processes. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2512_14238 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Revealing the baryon cycle in Galaxy Clusters: connecting galaxy dynamics and gas thermodynamics using (sub-)mm-wave and optical IFU surveys Montenegro-Montes, Francisco M. Sánchez-Blázquez, Patricia Mroczkowski, Tony de Paz, Armando Gil Catalán-Torrecilla, Cristina Gendron-Marsolais, Marie-Lou Macías-Pardo, Paula Callejas-Córdoba, Beatriz Montaña, Alfredo Macías-Pérez, Juan F. Planelles, Susana Cosmology and Nongalactic Astrophysics Observations in the visible and near infrared are transforming our view of the processes affecting galaxy evolution, much of which is dominated by interactions with the large scale environment. Yet a complete picture is missing, as no corresponding high resolution view of the warm/hot intracluster, circumgalactic, and intergalactic media exists over large areas and a comparably broad range of redshifts. Combined with wide-field optical IFU surveys such as CATARSIS, a large diameter sub-mm telescope with a degree-scale field of view would enable a joint view of galaxy dynamics and gas thermodynamics, transforming our understanding of environmental processes. |
| title | Revealing the baryon cycle in Galaxy Clusters: connecting galaxy dynamics and gas thermodynamics using (sub-)mm-wave and optical IFU surveys |
| topic | Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2512.14238 |