Strong, rare X-ray flares can temporarily increase gas-phase water abundance by factors of 3 to 13 at protoplanetary disk surfaces, with effects lasting days, while common weak flares do not produce observable changes.
A., Aikawa, Y., Blake, G
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Modeling Time Dependent Water Chemistry Due to Powerful X-ray Flares from T-Tauri Stars
Strong, rare X-ray flares can temporarily increase gas-phase water abundance by factors of 3 to 13 at protoplanetary disk surfaces, with effects lasting days, while common weak flares do not produce observable changes.