Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra I cluster: III. Untangling UDG 32 from the stripped filaments of NGC 3314A with multi-wavelength data

Context. UDG 32 is an ultra-diffuse galaxy (UDG) candidate in the Hydra I cluster that was discovered in the extended network of stellar filaments of the jellyfish galaxy NGC 3314A. This jellyfish galaxy is affected by ram pressure stripping and it is hypothesised that UDG 32 may have formed from th...

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Detalles Bibliográficos
Autores: Hartke, J., Iodice, E., Gullieuszik, M., Mirabile, M., Buttitta, C., Doll, G., D'Ago, G., de la Casa, C. C., Hess, Kelley M., Kotulla, Ralf, Poggianti, B., Arnaboldi, M., Cantiello, Michele, Corsini, E. M., Falcón-Barroso, Jesús, Forbes, Duncan A., Hilker, M., Mieske, S., Rejkuba, M., Spavone, M.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2025
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/386892
Acceso en línea:http://hdl.handle.net/10261/386892
Access Level:acceso abierto
Palabra clave:Galaxies: formation
Galaxies: clusters: individual: Hydra I
Galaxies: individual: UDG 32
Galaxies: individual: NGC 3314A
Descripción
Sumario:Context. UDG 32 is an ultra-diffuse galaxy (UDG) candidate in the Hydra I cluster that was discovered in the extended network of stellar filaments of the jellyfish galaxy NGC 3314A. This jellyfish galaxy is affected by ram pressure stripping and it is hypothesised that UDG 32 may have formed from this stripped material.

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