[HTML][HTML] H2 formation on interstellar dust grains: The viewpoints of theory, experiments, models and observations
Molecular hydrogen is the most abundant molecule in the universe. It is the first one to form
and survive photo-dissociation in tenuous environments. Its formation involves catalytic …
and survive photo-dissociation in tenuous environments. Its formation involves catalytic …
Turbulent molecular clouds
P Hennebelle, E Falgarone - The Astronomy and Astrophysics Review, 2012 - Springer
Stars form within molecular clouds but our understanding of this fundamental process
remains hampered by the complexity of the physics that drives their evolution. We review our …
remains hampered by the complexity of the physics that drives their evolution. We review our …
PDRs4All: A JWST early release science program on radiative feedback from massive stars
The James Webb Space Telescope (JWST, Gardner et al. 2006) is a 6.5 m space telescope
launched in 2021 December and is developed by the National Aeronautics and Space …
launched in 2021 December and is developed by the National Aeronautics and Space …
Evolution of polycyclic aromatic hydrocarbons in photodissociation regions-Hydrogenation and charge states
J Montillaud, C Joblin, D Toublanc - Astronomy & Astrophysics, 2013 - aanda.org
Context. Various studies have emphasised variations in the charge state and composition of
the interstellar polycyclic aromatic hydrocarbon (PAH) population in photodissociation …
the interstellar polycyclic aromatic hydrocarbon (PAH) population in photodissociation …
Surface chemistry in the interstellar medium-I. H2 formation by Langmuir-Hinshelwood and Eley-Rideal mechanisms
J Le Bourlot, F Le Petit, C Pinto, E Roueff… - Astronomy & …, 2012 - aanda.org
Context. It has been found from ISO, Spitzer, and Herschel observations that molecular
hydrogen, H 2, can form on warm grains. Numerical models of interstellar chemistry have …
hydrogen, H 2, can form on warm grains. Numerical models of interstellar chemistry have …
GOALS-JWST: Tracing AGN feedback on the star-forming interstellar medium in NGC 7469
Abstract We present James Webb Space Telescope (JWST) Mid-Infrared Instrument (MIRI)
integral-field spectroscopy of the nearby merging, luminous infrared galaxy, NGC 7469. This …
integral-field spectroscopy of the nearby merging, luminous infrared galaxy, NGC 7469. This …
Structure of photodissociation fronts in star-forming regions revealed by Herschel observations of high-J CO emission lines
Context. In bright photodissociation regions (PDR) associated with massive star formation,
the presence of dense “clumps” that are immersed in a less dense interclump medium is …
the presence of dense “clumps” that are immersed in a less dense interclump medium is …
H2 Formation on Interstellar Grains
G Vidali - Chemical reviews, 2013 - ACS Publications
The first detection of molecules in space (CH, CH+, and CN) occurred in the late 1930s.
Since then over 180 different molecular species have been detected (http://www …
Since then over 180 different molecular species have been detected (http://www …
Shock-enhanced C+ Emission and the Detection of H2O from the Stephan's Quintet Group-wide Shock Using Herschel
PN Appleton, P Guillard, F Boulanger… - The Astrophysical …, 2013 - iopscience.iop.org
We present the first Herschel spectroscopic detections of the [O i] 63 μm and [C ii] 158 μm
fine-structure transitions, and a single para-H 2 O line from the 35× 15 kpc 2 shocked …
fine-structure transitions, and a single para-H 2 O line from the 35× 15 kpc 2 shocked …
PDRs4All-II. JWST's NIR and MIR imaging view of the Orion Nebula
Context. The James Webb Space Telescope (JWST) has captured the most detailed and
sharpest infrared (IR) images ever taken of the inner region of the Orion Nebula, the nearest …
sharpest infrared (IR) images ever taken of the inner region of the Orion Nebula, the nearest …