Probing the filamentary nature of star formation in the California giant molecular cloud

TL;DR

This study investigates the filamentary structures in the California molecular cloud, revealing their crucial role in star formation and the origin of the stellar initial mass function through detailed analysis of cores and filaments.

Contribution

It provides new observational evidence linking filament properties to the stellar initial mass function, proposing a revised model for core formation within filaments.

Findings

Both the core mass function and filament line mass function follow power-law distributions.

Results support a direct connection between filament properties and the stellar initial mass function.

Filamentary structures are identified as key to the evolution of star-forming regions.

Abstract

Recent studies suggest that filamentary structures are representative of the initial conditions of star formation in molecular clouds and support a filament paradigm for star formation, potentially accounting for the origin of the stellar initial mass function (IMF). Using Herschel imaging observations of the California giant molecular cloud, we aim to further investigate the filament paradigm for low- to intermediate-mass star formation and to better understand the exact role of filaments in the origin of stellar masses. Using the multiscale, multiwavelength extraction method getsf, we identify starless cores, protostars, and filaments in the Herschel data set and separate these components from the background cloud contribution to determine accurate core and filament properties. Both the prestellar core mass function (CMF) and the distribution of filament masses per unit length or filament line mass function (FLMF) are consistent with power-law distributions at the high-mass end, $\Delta N/\Delta {\rm log}M\propto M^{-1.4 \pm 0.2}$ at $M > 1\,M_\odot$ for the CMF and $\Delta N/\Delta {\rm log} {M}_{\rm line} \propto {M}_{\rm line}^{-1.5\pm0.2}$ for the FLMF at $M_{\rm line} > 10\,M_\odot {\rm pc^{-1}}$, which are both consistent with the Salpeter power-law IMF. Based on these results, we propose a revised model for the origin of the CMF in filaments, whereby the global prestellar CMF in a molecular cloud arises from the integration of the CMFs generated by individual thermally supercritical filaments within the cloud. Our findings support the existence a tight connection between the FLMF and the CMF/IMF and suggests that filamentary structures represent a critical evolutionary step in establishing a Salpeter-like mass function.