activity
20162026
most citedParameterizing the interstellar dust temperature

69 citations · 110 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

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-…

astro-ph.GA2019★ 5 cited

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…

astro-ph.GA2017★ 11 cited

The first frost in the Pipe Nebula

Miwa Goto, J. D. Bailey, Seyit Hocuk +4

Spectroscopic studies of ices in nearby star-forming regions indicate that ice mantles form on dust grains in two distinct steps, starting with polar ice formation (H2O rich) and s…

astro-ph.GA2017★ 69 cited

Parameterizing the interstellar dust temperature

S. Hocuk, L. Szucs, P. Caselli +3

The temperature of interstellar dust particles is of great importance to astronomers. It plays a crucial role in the thermodynamics of interstellar clouds, because of the gas-dust…

astro-ph.GA2016★ 25 cited

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…