The DOI matches its Crossref record; 65 of the 65 references it cites were found in a registry or an index.
The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point
Open accessAbstract
Context. The evolution of amorphous hydrocarbon materials, a-C(:H), principally resulting from ultraviolet (UV) photon absorption-induced processing, are likely at the heart of the variations in the observed properties of dust in the interstellar medium.
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Citations
Cites
Interpretation of Raman spectra of disordered and amorphous carbon
Ferrari, A. C., & Robertson, J. (2000) · Physical Review B · doi:10.1103/physrevb.61.14095 · Cited by 15,651
Optical Properties and Electronic Structure of Amorphous Germanium
Tauc, J., Grigorovici, R., & Vancu, A. (1966) · physica status solidi (b) · doi:10.1002/pssb.19660150224 · Cited by 11,071
Robertson, J. (2002) · Materials Science and Engineering: R: Reports · doi:10.1016/s0927-796x(02)00005-0 · Cited by 6,206
The size distribution of interstellar grains
Mathis, J. S., Rumpl, W., & Nordsieck, K. H. (1977) · The Astrophysical Journal · doi:10.1086/155591 · Cited by 3,856
Optical properties of interstellar graphite and silicate grains
Draine, B. T., & Lee, H. M. (1984) · The Astrophysical Journal · doi:10.1086/162480 · Cited by 3,279
Raman spectroscopy of amorphous, nanostructured, diamond–like carbon, and nanodiamond
Ferrari, A. C., & Robertson, J. (2004) · Philosophical Transactions of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences · doi:10.1098/rsta.2004.1452 · Cited by 2,689
A survey of interstellar H I from L-alpha absorption measurements. II
Bohlin, R. C., Savage, B. D., & Drake, J. F. (1978) · The Astrophysical Journal · doi:10.1086/156357 · Cited by 2,540
Ordal, M. A., Long, L. L., Bell, R. J., Bell, S. E., Bell, R. R., Alexander, R. W., & Ward, C. A. (1983) · Applied Optics · doi:10.1364/ao.22.001099 · Cited by 2,136
Draine, B. T., & Li, A. (2007) · The Astrophysical Journal · doi:10.1086/511055 · Cited by 2,122
Low-Pressure, Metastable Growth of Diamond and "Diamondlike" Phases
Angus, J. C., & Hayman, C. C. (1988) · Science · doi:10.1126/science.241.4868.913 · Cited by 1,574
Cited by
Wakelam, V., Bron, E., Cazaux, S., Dulieu, F., Gry, C., Guillard, P., Habart, E., Hornekær, L., Morisset, S., Nyman, G., et al. (2017) · Molecular Astrophysics · doi:10.1016/j.molap.2017.11.001 · Cited by 267
Viaene, S., Baes, M., Tamm, A., Tempel, E., Bendo, G., Blommaert, J. A. D. L., Boquien, M., Boselli, A., Camps, P., Cooray, A., et al. (2017) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201629251 · Cited by 79
Metadata
- Authors
- Jones, A. P., Fanciullo, L., Köhler, M., Verstraete, L., Guillet, V., Bocchio, M., & Ysard, N.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2013-10
- Volume
- 558
- Pages
- A62
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2044189059
- Cited by
- 444
- References
- 65
- FWCI
- 18.41
- Type
- journal article
- Language
- en
- Open access
- bronze
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- CoChat. (2026). Citation check: The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point. https://app.cochat.ai/papers/10.1051/0004-6361/201321686
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- Jones, A. P., Fanciullo, L., Köhler, M., Verstraete, L., Guillet, V., Bocchio, M., & Ysard, N. (2013). The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/201321686
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
