Constraining the Diffusion Coefficient and Cosmic-Ray Acceleration Efficiency using Gamma-ray Emission from the Star-Forming Region RCW 38

TL;DR

This study uses gamma-ray observations of RCW 38 to estimate cosmic-ray acceleration efficiency from stellar winds, suggesting stellar winds can significantly contribute to Galactic cosmic rays.

Contribution

It provides the first detailed gamma-ray analysis of RCW 38 to constrain cosmic-ray acceleration efficiency from stellar winds, highlighting their potential role in Galactic cosmic-ray production.

Findings

Detected gamma-ray emission coincident with RCW 38 star cluster.

Estimated cosmic-ray acceleration efficiency of about 40%.

Found cosmic-ray pressure is negligible compared to hot gas pressure.

Abstract

Stellar winds from massive stars may be significant sources of cosmic rays (CRs). To investigate this connection, we report a detailed study of gamma-ray emission near the young Milky Way star cluster ($\approx$ 0.5 Myr old) in the star-forming region RCW 38 and compare this emission to its stellar wind properties and diffuse X-ray emission. Using 15 years of Fermi-LAT data in the 0.2 $-$ 300 GeV band, we find a significant ($ \sigma > 22$) detection coincident with the star cluster, producing a total $\gamma$-ray luminosity (extrapolated over 0.1 $-$ 500 GeV) of $L_{\gamma} = (2.66\pm 0.92) \times 10^{34}$ erg s$^{-1}$ adopting a power-law spectral model ($\Gamma = 2.34\pm0.04$). Using an empirical relationship and Starburst99, we estimate the total wind power to be $8 \times 10^{36}$ erg s$^{-1}$, corresponding to a CR acceleration efficiency of $\eta_{\rm CR} \simeq 0.4$ for an assumed diffusion coefficient consistent with $D = 10^{28}$ cm$^{2}$ s$^{-1}$. Alternatively, a lower acceleration efficiency of 0.1 can produce this $L_{\gamma}$ if the diffusion coefficient is smaller, $D\simeq 2.5\times10^{27}\,{\rm cm^2\,\,s^{-1}}$. Additionally, we analyze Chandra X-ray data from the region and compare the hot-gas pressure to the CR pressure. We find the former is four orders of magnitude greater, suggesting that the CR pressure is not dynamically important relative to stellar winds. As RCW 38 is too young for supernovae to have occurred, the high CR acceleration efficiency in RCW 38 demonstrates that stellar winds may be an important source of Galactic CRs.