![]() We aim to reveal the gas energetics in the circumstellar environment of the prototypical high-mass protostellar object AFGL 2591. ![]() To probe this, space-based far-infrared observations are required.Īims. Molecular gas in the environment of massive protostellar objects, however, is known to reach temperatures of several hundred K. For these species, temperatures of ≲ 50 K are sufficient to produce emission lines that are observable from the ground at (sub)millimeter wavelengths. Linear rotor molecules such as CO, HCO + and HCN are important probes of star-forming gas. de l’Observatoire, 75014 Paris, Franceĥ Laboratoire d’Astrophysique de Grenoble, UMR 5571-CNRS, Université Joseph Fourier, Grenoble, FranceĬontext. Ceccarelli 5ġ Kapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen, The NetherlandsĮ-mail: SRON Netherlands Institute for Space Research, PO Box 800, 9700 AV Groningen, The Netherlandsģ Institute for Space Imaging Science, Department of Physics & Astronomy, University of Lethbridge, Lethbridge AB, T1K 3M4, CanadaĤ LERMA, UMR 8112 du CNRS, Observatoire de Paris, 61, Av. Astronomical objects: linking to databases.Including author names using non-Roman alphabets.Suggested resources for more tips on language editing in the sciences Punctuation and style concerns regarding equations, figures, tables, and footnotes
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