Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
Next revision Both sides next revision
papers [2020/07/20 10:33]
al
papers [2020/07/30 17:16]
bg
Line 46: Line 46:
 E. Allys, F. Levrier, S. Zhang, C. Colling, B. Regaldo-Saint Blancard, F. Boulanger, P. Hennebelle, S. Mallat E. Allys, F. Levrier, S. Zhang, C. Colling, B. Regaldo-Saint Blancard, F. Boulanger, P. Hennebelle, S. Mallat
  
-A&A 629, 115, 2019+A&A 629, 115, (2019)
  
 [[https://​www.aanda.org/​articles/​aa/​pdf/​2019/​09/​aa34975-18.pdf|PDF]] [[https://​www.aanda.org/​articles/​aa/​pdf/​2019/​09/​aa34975-18.pdf|PDF]]
Line 86: 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 ==
Line 112: 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, ​MPérault, and M. Gerin+E. Bellomi, B. Godard, P. Hennebelle, V. Valdivia, ​GPineau des Forêts, P. Lesaffre, and M. Pérault
  
 A&A .... (2020) accepted A&A .... (2020) accepted
  • papers.txt
  • Last modified: 2022/01/20 11:18
  • by pl