ISO Spectroscopy of Gas and Dust: From Molecular Clouds to Protoplanetary Disks

By E. Dishoeck. 2004

236 citations recorded by the source corpus.

▪ Abstract Observations of interstellar gas-phase and solid-state species in the 2.4–200 μm range obtained with the spectrometers on board the Infrared Space Observatory (ISO) are reviewed. Lines a...

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/e23fad4909f067c618371bb748cc9e30a6208df8

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Citations in the corpus

Cold Dark Clouds: The Initial Conditions for Star Formation (2007, background): “…probes of physical conditions (Evans 1999), gas/dust chemistry and star formation (van Dishoeck and Blake 1998; Ehrenfreund and Charnley 2000; van Dishoeck 2004), and the entire Protostars and Planets V volume (Reipurth et al. 2007), especially the papers by Ceccarelli et al., Di Francesco et…”
Experimental evidence for water formation on interstellar dust grains by hydrogen and oxygen atoms (2009, background): “Part of this gas and dust grains, covered with icy mantles (mainly composed of water), ends upin the rotating disks surrounding young stars and forms the basic material from which icy planetesimals and later planets, together with comets in the external regions, are formed (van Dishoeck 2004).”
Formation of Complex Molecules in Prestellar Cores: A Multilayer Approach (2017, background): “…of observations over the last four decades revealed the main constituents of interstellar ices to be water (Gillett & Forrest 1973), carbon monoxide (Lacy et al. 1984), carbon dioxide (de Graauw et al. 6 1996), methanol (Grim et al. 1991), ammonia (van Dishoeck 2004) and methane (Lacy et al. 1991).”
Ice structures, patterns, and processes: A view across the icefields (2012, background): “Larger icy bodies are supposed to have formed through the accretion and reprocessing of this material (van Dishoeck, 2004; Ehrenfreund et al., 2003).”
THE NASA AMES POLYCYCLIC AROMATIC HYDROCARBON INFRARED SPECTROSCOPIC DATABASE: THE COMPUTED SPECTRA (2010, unknown): “…et al. 1973) and attributed to molecular-sized species by Sellgren (1984), is now generally attributed to polycyclic aromatic hydrocarbons (PAHs; e.g., Puget & Leger 1989; Allamandola et al. 1989; van Dishoeck 2004; Peeters et al. 2004a; Draine & Li 2007; Tielens 2008, and references therein).”
WFCAM, Spitzer/IRAC and SCUBA observations of the massive star-forming region DR21/W75 - I. The collimated molecular jets (2006, background): “…gSub-mm core coincides with Hii region W75N(B), which is further resolved into three UC Hii regions VLA1, VLA2, & VLA 3 (Torrelles et al. 1997). hFlux uncertain because this source is near the edge of the SCUBA map. ing [3.6]-[4.5] though reducing [5.8]-[8.0] (Gibb et al. 2000; van Dishoeck 2004).”
The Mid-infrared Instrument for JWST and Its In-flight Performance (2023, background): “Thus, penetrating cold cloud cores and other heavily obscured environments can be done much more thoroughly from space than from the ground (e.g., van Dishoeck 2004).”
A UNIFIED REPRESENTATION OF GAS-PHASE ELEMENT DEPLETIONS IN THE INTERSTELLAR MEDIUM (2009, background): “Other simple oxygen-bearing molecules in solid form, such as CO, CO2 and O2 generally have smaller abundances than that of H2O, but they are not entirely negligible (van Dishoeck 2004).”