Signatures of UV radiation in low-mass protostars I. Origin of HCN and CN emission in the Serpens Main region
A. Mirocha,
A. Karska,
M. Gronowski
et al.
Abstract:Context. Ultraviolet radiation (UV) influences the physics and chemistry of star-forming regions, but its properties and significance in the immediate surroundings of low-mass protostars are still poorly understood. Aims. We aim to extend the use of the CN/HCN ratio, already established for high-mass protostars, to the low-mass regime to trace and characterize the UV field around low-mass protostars on ∼ 0.6 × 0.6 pc scales. Methods. We present 5 × 5 maps of the Serpens Main Cloud encompassing 10 protostars ob… Show more
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