Differences
This shows you the differences between two versions of the page.
| Both sides previous revision Previous revision Next revision | Previous revision Next revision Both sides next revision | ||
|
papers [2020/07/18 15:09] ef |
papers [2020/07/30 17:16] bg |
||
|---|---|---|---|
| Line 25: | Line 25: | ||
| ApJ 871, 17 (2019) | ApJ 871, 17 (2019) | ||
| - | |||
| - | [[https://iopscience.iop.org/article/10.3847/1538-4357/aaf582|PDF]] | ||
| [[https://iopscience.iop.org/article/10.3847/1538-4357/aaf582/pdf|PDF]] | [[https://iopscience.iop.org/article/10.3847/1538-4357/aaf582/pdf|PDF]] | ||
| Line 44: | Line 42: | ||
| [[https://arxiv.org/pdf/1903.03131.pdf|PDF]] | [[https://arxiv.org/pdf/1903.03131.pdf|PDF]] | ||
| + | |||
| + | == - The RWST, a comprehensive statistical description of the non-Gaussian structures in the ISM == | ||
| + | E. Allys, F. Levrier, S. Zhang, C. Colling, B. Regaldo-Saint Blancard, F. Boulanger, P. Hennebelle, S. Mallat | ||
| + | |||
| + | A&A 629, 115, (2019) | ||
| + | |||
| + | [[https://www.aanda.org/articles/aa/pdf/2019/09/aa34975-18.pdf|PDF]] | ||
| == - Probing the cold magnetised Universe with SPICA-POL (B-BOP) == | == - Probing the cold magnetised Universe with SPICA-POL (B-BOP) == | ||
| Line 81: | Line 86: | ||
| [[https://academic.oup.com/mnras/article/495/1/816/5841083|PDF]] | [[https://academic.oup.com/mnras/article/495/1/816/5841083|PDF]] | ||
| + | |||
| + | == - Molecule formation in dust-poor irradiated jets. I. Stationary disk winds == | ||
| + | B. Tabone, B. Godard, G. Pineau des Forêts, S. Cabrit, and E. F. van Dishoeck | ||
| + | |||
| + | A&A 636, 60 (2020) | ||
| + | |||
| + | [[https://www.aanda.org/articles/aa/pdf/2020/04/aa37383-19.pdf|PDF]] | ||
| == - Self-generated ultraviolet radiation in molecular shock waves I. Effects of Lyman α, Lyman β and 2-photon continuum == | == - Self-generated ultraviolet radiation in molecular shock waves I. Effects of Lyman α, Lyman β and 2-photon continuum == | ||
| A. Lehmann, B. Godard, G. Pineau des Forêts, and E. Falgarone | A. Lehmann, B. Godard, G. Pineau des Forêts, and E. Falgarone | ||
| - | A&A ... (2020) | + | A&A (submitted) |
| == - Magnetic fields from multiplicative chaos == | == - Magnetic fields from multiplicative chaos == | ||
| Line 107: | Line 119: | ||
| == - 3-dimensional Chemical Structure of Diffuse Turbulent Interstellar Medium == | == - 3-dimensional Chemical Structure of Diffuse Turbulent Interstellar Medium == | ||
| - | E. Bellomi, B. Godard, P. Hennebelle, V. Valdivia, M. Pérault, and M. Gerin | + | E. Bellomi, B. Godard, P. Hennebelle, V. Valdivia, G. Pineau des Forêts, P. Lesaffre, and M. Pérault |
| A&A .... (2020) accepted | A&A .... (2020) accepted | ||
| + | |||
| + | == - Statistical description of dust polarized emission from the diffuse interstellar medium -- A WST/RWST approach == | ||
| + | B. Regaldo-Saint Blancard, F. Levrier, E. Allys, E. Bellomi, F. Boulanger | ||
| + | |||
| + | A&A ... (2020) accepted | ||
| + | |||
| + | [[https://arxiv.org/pdf/2007.08242.pdf|PDF]] | ||