CARMENES input catalogue of M dwarfs: IX. Multiplicity from close spectroscopic binaries to ultra-wide systems

[Context] Multiplicity studies greatly benefit from focusing on M dwarfs because they are often paired in a variety of configurations with both stellar and substellar objects, including exoplanets.

Bibliographic Details
Authors: Cifuentes, C., Caballero, J. A., González-Payo, J., Amado, Pedro J., Béjar, Victor J. S., Burgasser, Adam J., Cortés-Contreras, M., Lodieu, Nicolas, Montes, David, Quirrenbach, Andreas, Reiners, Ansgar, Ribas, Ignasi, Sanz-Forcada, J., Seifert, W., Zapatero Osorio, María Rosa
Format: article
Status:Published version
Publication Date:2025
Country:España
Institution:Consejo Superior de Investigaciones Científicas (CSIC)
Repository:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/385107
Online Access:http://hdl.handle.net/10261/385107
https://api.elsevier.com/content/abstract/scopus_id/85216195682
Access Level:Open access
Keyword:Astronomical databases: miscellaneous
Binaries: general
Stars: late-type
Virtual observatory tools
Description
Summary:[Context] Multiplicity studies greatly benefit from focusing on M dwarfs because they are often paired in a variety of configurations with both stellar and substellar objects, including exoplanets.

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