The dense cores and filamentary structure of the molecular cloud in Corona Australis. Herschel SPIRE and PACS observations from the Herschel Gould Belt Survey

TL;DR

This study catalogs prestellar and starless cores in the Corona Australis molecular cloud using Herschel data, revealing that higher-mass cores predominantly form on filaments, supporting the filamentary core formation paradigm.

Contribution

It provides the first comprehensive catalog of dense cores in Corona Australis and analyzes their spatial and mass distribution in relation to filamentary structures.

Findings

Higher-mass prestellar cores are located on or near filaments.

Lower-mass starless cores are found away from filaments.

The Coronet region shows signs of advanced evolutionary stage.

Abstract

We present a catalogue of prestellar and starless cores within the Corona Australis molecular cloud using photometric data from the Herschel Space Observatory. At a distance of d~130 pc, Corona Australis is one of the closest star-forming regions. Herschel has taken multi-wavelength data of Corona Australis with both the SPIRE and PACS photometric cameras in a parallel mode with wavelengths in the range 70 {\mu}m to 500 {\mu}m. A complete sample of starless and prestellar cores and embedded protostars is identified. Other results from the Herschel Gould Belt Survey have shown spatial correlation between the distribution of dense cores and the filamentary structure within the molecular clouds. We go further and show correlations between the properties of these cores and their spatial distribution within the clouds, with a particular focus on the mass distribution of the dense cores with respect to their filamentary proximity. We find that only lower-mass starless cores form away from filaments, while all of the higher-mass prestellar cores form in close proximity to, or directly on the filamentary structure. This result supports the paradigm that prestellar cores mostly form on filaments. We analyse the mass distribution across the molecular cloud, finding evidence that the region around the Coronet appears to be at a more dynamically advanced evolutionary stage to the rest of the clumps within the cloud.