Multiplicity of Cool Stars and their Evolution
Abstract
Making up a sizeable portion of the galactic census, stellar multiples are experiencing a renaissance. Enabling the study of multiple strands of the study of cool stars, stellar multiples have been found and characterised in great numbers by the missions of the last decade, allowing the exploration of stellar parameters and populations, observation of stellar interactions, studies into stellar formation and evolution, and characterisation of circumbinary systems. This exciting explosion of science is only set to continue, with future missions set to offer even further insights into the topic. Within these proceedings we will summarise the presentations and discussions on cool stellar multiplicity within our splinter sessions at the 23rd Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, as we examine the present state of the field and look to what the future may bring.
Versions
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BibTeX
@misc{swayne2026multiplicity,
title = {{Multiplicity of Cool Stars and their Evolution}},
author = {Matthew I. Swayne and Leen Decin and Theo Khouri and Ayush Moharana and Léa Planquart and John Southworth and Nikki J. Miller and José A. Caballero and Orsolo De Marco and Krzysztof G. Hełminiak and Swetlana Hubrig and Valentin D. Ivanov and Pierre Kervella and Thibault Merle and Dorota M. Skowron},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.02400},
eprint = {2609.02400},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.02400},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Multiplicity of Cool Stars and their Evolution
AU - Matthew I. Swayne
AU - Leen Decin
AU - Theo Khouri
AU - Ayush Moharana
AU - Léa Planquart
AU - John Southworth
AU - Nikki J. Miller
AU - José A. Caballero
AU - Orsolo De Marco
AU - Krzysztof G. Hełminiak
AU - Swetlana Hubrig
AU - Valentin D. Ivanov
AU - Pierre Kervella
AU - Thibault Merle
AU - Dorota M. Skowron
PY - 2026
DA - 2026/09/02
PB - arXiv
DO - 10.48550/arxiv.2609.02400
UR - https://arxiv.org/abs/2609.02400
AB - Making up a sizeable portion of the galactic census, stellar multiples are experiencing a renaissance. Enabling the study of multiple strands of the study of cool stars, stellar multiples have been found and characterised in great numbers by the missions of the last decade, allowing the exploration of stellar parameters and populations, observation of stellar interactions, studies into stellar formation and evolution, and characterisation of circumbinary systems. This exciting explosion of science is only set to continue, with future missions set to offer even further insights into the topic. Within these proceedings we will summarise the presentations and discussions on cool stellar multiplicity within our splinter sessions at the 23rd Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, as we examine the present state of the field and look to what the future may bring.
ER -