Interstellar Ice: The Infrared Space Observatory Legacy

By E. Gibb, D. Whittet, A. Boogert, A. Tielens. 2004

697 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/c87d40f29033b6232258f63fa5e150d9da7bffee

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. R. Garrod
2. E. Dishoeck
3. P. Caselli
4. N. Evans II
5. K. Oberg
6. E. Bergin
7. E. Herbst
8. P. Myers

In Atomic and Molecular Physics, and Optics

1. R. Garrod
2. E. Dishoeck
3. E. V. van Dishoeck
4. Ralf I. Kaiser
5. A. Tielens
6. K. Oberg
7. H. Linnartz
8. P. Caselli

In Spectroscopy

1. R. Garrod
2. E. Dishoeck
3. P. Caselli
4. K. Oberg
5. E. Herbst
6. E. V. van Dishoeck
7. A. Tielens
8. E. Bergin

Citations in the corpus

• The Wavelength Dependence of Interstellar Extinction from 1.25 to 8.0 μm Using GLIMPSE Data (2004, background): “The ISO spectra of heavily obscured objects in Gibb et al. (2004) show 8 m fluxes that seem little affected by silicate absorption.”
• Microscopic simulation of methanol and formaldehyde ice formation in cold dense cores (2009, methodology): “These detections occur mostly in high-mass young stellar sources such as W33A, GL2136, and GL 989, and often only upper limits are given (Boogert et al. 2008; Gibb et al. 2004).”
• Formation of Complex Molecules in Prestellar Cores: A Multilayer Approach (2017, background): “A three-phase code with bulk chemistry In cold dark clouds, the thickness of icy mantles on interstellar grains is significant, and reach up to several hundreds monolayers (e.g., Gibb et al. 2004; Garrod & Pauly 2011; Vasyunin & Herbst 2013a).”
• H-atom addition and abstraction reactions in mixed CO, H2CO and CH3OH ices – an extended view on complex organic molecule formation (2016, background): “…show that rather than mixing with H2O, the bulk of the CO accretes on top of a previously formed H2O-rich polar ice, forming an apolar COrich ice layer (Tielens et al. 1991, Öberg et al. 2011a; Boogert & Ehrenfreund 2004; Gibb et al. 2004; Mathews et al. 2013, Boogert, Gerakines & Whittet 2015).”
• Formation rates of complex organics in UV irradiated CH3OH-rich ices I: Experiments (2009, background): “More complex ices have been ten- tatively detected towards a few high-mass protostars (Schutte et al. 1999; Gibb et al. 2004), though specific band assignments are uncertain.”
• Testing grain-surface chemistry in massive hot-core regions (2007, background): “However, the high ice abundances of CH3OH (e.g., Gibb et al. 2004) and the constant abundance ratio between H2CO/CH3OH in this paper are inconsistent with this CH3OH destruction mechanism.”
• Observations of the Icy Universe (2015, methodology): “We refer to reviews by Gibb et al. (2004), Boogert & Ehrenfreund (2004b), and Dartois (2005) for historical work.”
• Water and astrobiology (2007, methodology): “A survey of 23 infrared sources by Gibb et al. (2004) using the Infrared Space Observatory found large discrepancies in the methanol abundance derived, in particular, when the 3.53 mm (2828 cm 1[C–”
• Complex Chemistry in Star-forming Regions: An Expanded Gas-Grain Warm-up Chemical Model (2008, background): “Infrared observations indicate the presence of icy grain mantles in the cold outer envelopes of protostellar objects (Gibb et al. 2004); these mantles are typically comprised mainly of H2O, CO and CO2.”
• Mechanistical Studies on the Irradiation of Methanol in Extraterrestrial Ices (2007, methodology): “A recent survey of 23 infrared sources carried out by Gibb et al. (2004) using the Infrared Space Observatory (ISO) found large discrepancies for the derived methanol abundance reported, in particular, between when the 3.53 m (2828 cm 1 [ 3, C-H stretch]) and 3.95 m (2531 cm 1 [ 6+ 11, combination…”
• THE MID-INFRARED EXTINCTION LAW IN THE OPHIUCHUS, PERSEUS, AND SERPENS MOLECULAR CLOUDS (2008, methodology): “0 dust model incorporates the 6.02 µm water ice absorption line (Gibb et al. 2004), which is within the IRAC 5.8 µm bandpass.”
• Cold Dark Clouds: The Initial Conditions for Star Formation (2007, background): “Icy mantles coating grains in ambient gas are dominated by H2O ice with substantial amounts of CO and CO2 at a level of ∼25% of the water ice abundance in each case (Gibb et al. 2004).”
• NON-RACEMIC AMINO ACID PRODUCTION BY ULTRAVIOLET IRRADIATION OF ACHIRAL INTERSTELLAR ICE ANALOGS WITH CIRCULARLY POLARIZED LIGHT (2011, background): “Ices are widely observed in many astrophysical environments (Gibb et al. 2004; Dartois 2005), particularly in dense molecular protostellar clouds from which stars, disks, debris such as asteroids and comets, and eventually planetary systems form.”
• Infrared Extinction toward Nearby Star-forming Regions (2007, background): “Dust in molecular cloud cores is protected both from the UV interstellar radiation field and from cosmic ray processing; those dust grains may therefore have larger mantles consisting of water and organic ices (Gibb et al. 2004).”
• Mechanisms of Amino Acid Formation in Interstellar Ice Analogs (2007, background): “However, specific environments and compositions of ices within such clouds will, of course, vary over a range (Gibb et al. 2004).”