H$$_2$$ Formation on Interstellar Dust Grains: The Viewpoints of Theory, Experiments, Models and Observations
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Publisher
Springer International Publishing
Link
https://link.springer.com/content/pdf/10.1007/978-3-031-29003-9_16
Reference37 articles.
1. Alata, I., Cruz-Diaz, G.A., Muñoz Caro, G.M. et al.: Vacuum ultraviolet photolysis of hydrogenated amorphous carbons - I. Interstellar H$$_2$$ and ch4 formation rates. A&A 569, A119 (2014). https://doi.org/10.1051/0004-6361/201323118
2. Andrews, H., Candian, A., Tielens, A.G.G.M.: Hydrogenation and dehydrogenation of interstellar PAHs: Spectral characteristics and H$$_2$$ formation. A&A 595, A23 (2016); https://doi.org/10.1051/0004-6361/201628819
3. Arab, H., Abergel, A., Habart, E., et al. : Evolution of dust in the Orion Bar with Herschel - I. Radiative transfer modelling. A&A 541, A19 (2012). https://doi.org/10.1051/0004-6361/201118537
4. Berné, O., Joblin, C., Deville, Y., et al.: Analysis of the emission of very small dust particles from spitzer spectro-imagery data using blind signal separation method. A&A 469(2), 575–586 (2007). https://doi.org/10.1051/0004-6361:20066282
5. Boschman, L., Cazaux, S., Spaans, M., et al.: H$$_2$$ formation on PAHs in photodissociation regions: a high-temperature pathway to molecular hydrogen. A&A 579, A72 (2015); https://doi.org/10.1051/0004-6361/201323165
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