... The State of the Gas and the Relation between Gas and Star Formation at Low Metallicity: The Small Magellanic Cloud . ... We compare atomic gas, molecular gas, and the recent star formation rate (SFR) inferred from HЮБ in the Small Magellanic Cloud ...
... of dust grains and the subsequent dust emissivity increase in molecular clouds, and/or accretion of gas-phase metals onto dust grains, and the subsequent dust abundance (dust-to-gas ratio) increase in molecular clouds could explain the observations ...
... Space Telescope Science Institute . Gas Flows in Galaxies . 2012 STScI May Symposium: . ... 2012 STScI May Symposium: . Gas Flows in Galaxies: May 7-10, 2012 . Invited Speakers . Scientific Organizing Committee. ...
... The Herschel Exploitation of Local Galaxy Andromeda (HELGA). II. Dust and Gas in Andromeda . ... We present an analysis of the dust and gas in Andromeda, using Herschel images sampling the entire far-infrared peak. ...
... Dust and Atomic Gas in Dwarf Irregular Galaxies of the M81 Group: The SINGS and THINGS View . ... show distinctly different spectral shapes and aromatic features, although the galaxies have comparable gas-phase metallicities ...
... Interstellar gas, dust and diffuse bands in the SMC . ... DIBs, and physical and chemical conditions of the diffuse interstellar medium (gas and dust) in the Small Magellanic Cloud (SMC ...
... The SAGE-Spec Spitzer Legacy Program: The Life Cycle of Dust and Gas in the Large Magellanic Cloud . ... The SAGE-Spec program aims to study the life cycle of gas and dust in the Large Magellanic Cloud and to provide information ...
... Physical Conditions in the Ionized Gas of 30 Doradus . ... moderately ionized species of argon, neon, and sulfur, which are used to determine the physical conditions in the ionized gas ...