Velocity-resolved [O I] maps of the Orion BN/KL outflow yield a total luminosity of 86.5 L_sun and line ratios indicating dense (10^5–10^6 cm^-3), warm (~500 K) postshock gas from 30–40 km/s dissociative J-type shocks illuminated by external UV.
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Shiva is a new simulation tool that computes time-dependent dust size distributions and band gap energy evolution for HAC grains under photo-processing, sputtering, and shattering in specified interstellar conditions.
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Velocity-resolved [O I] 63,145 um, [C II] 158 um, and OH line mapping along the Orion BN/KL explosive outflow and irradiated shocks
Velocity-resolved [O I] maps of the Orion BN/KL outflow yield a total luminosity of 86.5 L_sun and line ratios indicating dense (10^5–10^6 cm^-3), warm (~500 K) postshock gas from 30–40 km/s dissociative J-type shocks illuminated by external UV.
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Shiva: the dust destruction model
Shiva is a new simulation tool that computes time-dependent dust size distributions and band gap energy evolution for HAC grains under photo-processing, sputtering, and shattering in specified interstellar conditions.