5 citations · 5 across the 2 of their papers we have counts for
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Class I CH3OH Maser Emission from Bar-Driven Inflow Colliding with the Central Molecular Zone
V. S. Veena, W. -J. Kim, P. Schilke +9
The Central Molecular Zone of the Milky Way is shaped by the interplay of bar-driven inflows, shocks, and star formation. At Galactic longitude l=1.3, gas inflowing along the near-…
Dust temperature and time-dependent effects in the chemistry of photodissociation regions
Gisela Esplugues, Stephanie Cazaux, Paola Caselli +2
When studying the chemistry of PDRs, time dependence becomes important as visual extinction increases, since certain chemical timescales are comparable to the cloud lifetime. Dust…
Surface chemistry in photodissociation regions
G. B. Esplugues, S. Cazaux, R. Meijerink +2
The presence of dust can strongly affect the chemical composition of the interstellar medium. We model the chemistry in photodissociation regions (PDRs) using both gas-phase and du…