Physics of ULIRGs with MUSE and ALMA: The PUMA project: I. Properties of the survey and first MUSE data results

Physics of ULIRGs with MUSE and ALMA: The PUMA project: I. Properties of the survey and first MUSE data results

Context. Ultraluminous infrared galaxies (ULIRGs) are characterised by extreme starburst (SB) and active galactic nucleus (AGN) activity, and are therefore ideal laboratories for studying the outflow phenomena and their feedback effects. We have recently started a project called Physics of ULIRGs wi...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2021-02, Vol.646, p.A101
Hauptverfasser: Perna, M., Arribas, S., Pereira Santaella, M., Colina, L., Bellocchi, E., Catalán-Torrecilla, C., Cazzoli, S., Crespo Gómez, A., Maiolino, R., Piqueras López, J., Rodríguez del Pino, B.
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Sprache:eng
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Zusammenfassung:Context. Ultraluminous infrared galaxies (ULIRGs) are characterised by extreme starburst (SB) and active galactic nucleus (AGN) activity, and are therefore ideal laboratories for studying the outflow phenomena and their feedback effects. We have recently started a project called Physics of ULIRGs with MUSE and ALMA (PUMA), which is a survey of 25 nearby ( z  
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361/202039702