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Blowing star formation away in Active galactic nuclei Hosts

The BAH Project aims to explore the intricate processes of AGN feeding and feedback through a multiwavelength observations. By focusing on nearby Active Galactic Nuclei (AGN) hosts with strong molecular hydrogen emission, the project seeks to unveil the mechanisms driving gas inflow (feeding) and the subsequent impact of AGN-driven outflows (feedback) on their host galaxies.

TEAM
Rogemar A. Riffel (UFSM - Brazil)
Marina Bianchin (UCI - USA)
Nadia L. Zakamska (JHU - USA)
Rogério Riffel (UFRGS - Brazil)
Thaisa Storchi-Bergmann (UFRGS - Brazil)
 
Gabriel Luan Souza-Oliveira (UFSM - Brazil)
José Henrique Costa-Souza (UFSM - Brazil)
Lucas Ramos Vieira (UFSM - Brazil)

Maitê S. de Zorzi de Mellos (UFSM - Brazil)

 

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