Runaway stars as cosmic ray injectors inside molecular clouds

Abstract

Giant molecular clouds (GMCs) are a new population of gamma-ray sources, being the target of cosmic rays (CRs) -- locally accelerated or not --. These clouds host very young stellar clusters where massive star formation takes place. Eventually, some of the stars are ejected from the clusters, becoming runaway stars. These stars move supersonically through the cloud and develop bowshocks where particles can be accelerated up to relativistic energies. As a result, the bowshocks present non-thermal emission, and inject relativistic protons in the cloud. These protons diffuse in the GMC interacting with the matter. We present a model for the non-thermal radiation generated by protons and secondary pairs accelerated in the bowshocks of massive runaways stars within young GMCs. We solve the transport equation for primary protons and secondary pairs as the stars move through the cloud. We present non-thermal emissivity maps in radio and in gamma rays as a function of time. We obtain X-ray luminosities of the order $\sim$ $10^{32}$ erg~s${}^{-1}$ and gamma-ray luminosities $\sim$ $10^{34}$ erg~s${}^{-1}$. We conclude that, under some assumptions, relativistic protons from massive runaway stars interacting with matter in GMCs give rise to extended non-thermal sources.

16 pages, 10 figures, accepted for publication in MNRAS

References in corpus (5)

• Cosmic Ray Propagation: Nonlinear Diffusion Parallel and Perpendicular to Mean Magnetic Field
• The VLT-FLAMES Tarantula Survey III: A very massive star in apparent isolation from the massive cluster R136
• Leptonic secondary emission in a hadronic microquasar model
• Gamma-ray observations of the Orion Molecular Clouds with the Fermi Large Area Telescope
• Cosmic Ray transport through gyroresonance instability in compressible turbulence

Cited by in corpus (5)

• Bow shock nebulae of hot massive stars in a magnetized medium
• Wind nebulae and supernova remnants of very massive stars
• Magnetic Field Orientation in Self-Gravitating Turbulent Molecular Clouds
• Searching for Faint X-ray Emission from Galactic Stellar Wind Bow Shocks
• Non-thermal emission in hyper-velocity and semi-relativistic stars