Corona-Australis is one of the nearest regions to the Sun with active star formation, but despite the close proximity (d~150 pc) our current picture of this starburst is not yet complete. Our team has recently revised the census of Corona-Australis stars using Gaia- DR2 data and discovered a distributed population of young stars located in the Galactic north of the dark clouds that is twice as numerous as the historically known stellar population concentrated around the densest cores of the region. Here, we build on the current census of stars in this region by combining the Gaia-EDR3 catalogue with astrometric and photometric ground-based data delivered by the Cosmic-DANCe project. We use our new sample of members and high-resolution spectroscopy to revisit the structure and kinematics of the Corona-Australis star-forming region.
{"references":["Blanco-Cuaresma et al. (2014), A&A 569, A111","Bouy et al. (2013), A&A 554, 101","Gaia Collaboration et al. (2021), A&A 650, C3","Galli et al. (2020), A&A 634, A98","Olivares et al. (2018), A&A 617, A15","Olivares et al. (2021), A&A 649, A159"]}