Radio survey of the stellar population in the infrared dark cloud G14.225-0.506

[Context] The infrared dark cloud (IRDC) G14.225-0.506 is part of the extended and massive molecular cloud located to the southwest of the H II region M17. The cloud is associated with a network of filaments, which result in two different dense hubs, as well as with several signposts of star formati...

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Bibliographic Details
Authors: Díaz-Márquez, Elena, Grau, Roger, Busquet, Gemma, Girart, Josep Miquel, Sánchez-Monge, Álvaro, Palau, Aina, Povich, Matthew S., Añez-López, N., Liu, Hauyu Baobab, Zhang, Qizhou, Estalella, Robert
Format: article
Status:Published version
Publication Date:2024
Country:España
Institution:Consejo Superior de Investigaciones Científicas (CSIC)
Repository:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/358069
Online Access:http://hdl.handle.net/10261/358069
Access Level:Open access
Keyword:Stars: formation
ISM: jets and outflows
Radio continuum: ISM
ISM: individual objects: G14.225-0.506
Description
Summary:[Context] The infrared dark cloud (IRDC) G14.225-0.506 is part of the extended and massive molecular cloud located to the southwest of the H II region M17. The cloud is associated with a network of filaments, which result in two different dense hubs, as well as with several signposts of star formation activity and a rich population of protostars and young stellar objects (YSOs).

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