PRODIGE – planet-forming disks in Taurus with NOEMA

[Context]: The physics and chemistry of planet-forming disks are far from being fully understood. To make further progress, both broad line surveys and observations of individual tracers in a statistically significant number of disks are required.

Detalhes bibliográficos
Autores: Semenov, A., Henning, Thomas, Guilloteau, S., Smirnov-Pinchukov, G., Dutrey, A., Chapillon, E., Piétu, V., Franceschi, R., Schwarz, K., Terwisga, S. van, Bouscasse, L., Caselli, P., Ceccarelli, C., Cunningham, N., Fuente, Asunción, Gieser, C., Hsieh, T.-H., López-Sepulcre, A., Segura-Cox, Dominique, Pineda, Jaime E., Maureira, M. J., Möller, T., Tafalla, M., Valdivia-Mena, M. T.
Tipo de documento: artigo
Estado:Versão publicada
Data de publicação:2024
País:España
Recursos:Consejo Superior de Investigaciones Científicas (CSIC)
Repositório:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/369689
Acesso em linha:http://hdl.handle.net/10261/369689
Access Level:Acceso aberto
Palavra-chave:Line: profiles
Techniques: interferometric
Protoplanetary disks
Stars: variables: T Tauri, Herbig Ae/Be
Radio lines: planetary systems
Descrição
Resumo:[Context]: The physics and chemistry of planet-forming disks are far from being fully understood. To make further progress, both broad line surveys and observations of individual tracers in a statistically significant number of disks are required.

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