Neutral hydrogen filaments in interstellar media: Are they physical?
Author:
Funder
Los Alamos National Laboratory
Publisher
Springer Science and Business Media LLC
Link
https://link.springer.com/content/pdf/10.1007/s41614-024-00156-5.pdf
Reference182 articles.
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2. B.G. Andersson, A. Lazarian, J.E. Vaillancourt, Interstellar dust grain alignment. ARA &A 53, 501–539 (2015). https://doi.org/10.1146/annurev-astro-082214-122414
3. P. André, J. Di Francesco, D. Ward-Thompson, et al. From filamentary networks to dense cores in molecular clouds: toward a new paradigm for star formation. In: Beuther H, Klessen RS, Dullemond CP, et al (eds) Protostars and Planets VI, pp. 27–51 (2014). https://doi.org/10.2458/azu_uapress_9780816531240-ch002. arXiv:1312.6232
4. D. Arzoumanian, P. André, V. Könyves et al., Characterizing the properties of nearby molecular filaments observed with Herschel. A &A 621, A42 (2019). https://doi.org/10.1051/0004-6361/201832725. arXiv:1810.00721 [astro-ph.GA]
5. E. Audit, P. Hennebelle, Thermal condensation in a turbulent atomic hydrogen flow. A &A 433(1), 1–13 (2005). https://doi.org/10.1051/0004-6361:20041474. arXiv:astro-ph/0410062 [astro-ph]
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