Red Supergiants -- The Other Side of the H-R Diagram
Fuente:
arXiv
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| Autore principale: | |
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| Natura: | Preprint |
| Pubblicazione: |
2025
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| _version_ | 1866913952163692544 |
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| author | Humphreys, Roberta M. |
| author_facet | Humphreys, Roberta M. |
| contents | Red supergiants are the largest stars known with some of the highest mass loss rates observed. They are the final stage in the evolution of the majority of massive stars. The unexpected discovery of high mass loss episodes in many red supergiants have posed questions about the role of mass loss on their final stages. The papers in this volume are timely reviews of our current understanding of this often surprising population of massive stars. This introductory paper is a brief summary of their observed properties and a historical perspective on some of the current problems on mass loss, their circumstellar environments, and their evolutionary state. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2507_15965 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Red Supergiants -- The Other Side of the H-R Diagram Humphreys, Roberta M. Solar and Stellar Astrophysics Red supergiants are the largest stars known with some of the highest mass loss rates observed. They are the final stage in the evolution of the majority of massive stars. The unexpected discovery of high mass loss episodes in many red supergiants have posed questions about the role of mass loss on their final stages. The papers in this volume are timely reviews of our current understanding of this often surprising population of massive stars. This introductory paper is a brief summary of their observed properties and a historical perspective on some of the current problems on mass loss, their circumstellar environments, and their evolutionary state. |
| title | Red Supergiants -- The Other Side of the H-R Diagram |
| topic | Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2507.15965 |