Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Pierre Palud"'
Autor:
Pierre Palud, Pierre Chainais, Franck Le Petit, Emeric Bron, Pierre-Antoine Thouvenin, Maxime Vono, L. Einig, M. Garcia Santa-Maria, M. Gaudel, J. H. Orkisz, V. de Souza Magalhaes, S. Bardeau, M. Gerin, J. R. Goicoechea, P. Gratier, V. V. Guzman, J. Kainulainen, F. Levrier, N. Peretto, J. Pety, A. Roueff, A. Sievers
Publikováno v:
2022 30th European Signal Processing Conference (EUSIPCO).
Autor:
Mathilde Gaudel, Jan H. Orkisz, Maryvonne Gerin, Jérôme Pety, Antoine Roueff, Antoine Marchal, François Levrier, Marc-Antoine Miville-Deschênes, Javier R. Goicoechea, Evelyne Roueff, Franck Le Petit, Victor de Souza Magalhaes, Pierre Palud, Miriam G. Santa-Maria, Maxime Vono, Sébastien Bardeau, Emeric Bron, Pierre Chainais, Jocelyn Chanussot, Pierre Gratier, Viviana Guzman, Annie Hughes, Jouni Kainulainen, David Languignon, Jacques Le Bourlot, Harvey Liszt, Karin Öberg, Nicolas Peretto, Albrecht Sievers, Pascal Tremblin
Publikováno v:
Astronomy & Astrophysics. 670:A59
39 pags., 78 figs., 2 tabs. 6 apps.
Understanding the initial properties of star-forming material and how they affect the star formation process is key. From an observational point of view, the feedback from young high-mass stars on future star
Understanding the initial properties of star-forming material and how they affect the star formation process is key. From an observational point of view, the feedback from young high-mass stars on future star
Autor:
Emeric Bron, Evelyne Roueff, Maryvonne Gerin, Jérôme Pety, Pierre Gratier, Franck Le Petit, Viviana Guzman, Jan Orkisz, Victor de Souza Magalhaes, Mathilde Gaudel, Pierre Palud, Lucas Einig, Sébastien Bardeau, Pierre Chainais, Jocelyn Chanussot, Javier Goicoechea, Annie Hughes, Jouni Kainulainen, David Languignon, Jacques Le Bourlot, François Levrier, Darek Lis, Harvey Liszt, Karin Öberg, Nicolas Peretto, Antoine Roueff, Albrecht Sievers, Pierre-Antoine Thouvenin, Pascal Tremblin
Publikováno v:
EPJ Web of Conferences. 265:00023
The ionization fraction in neutral interstellar clouds is a key physical parameter controlling multiple physical and chemical processes, and varying by orders of magnitude from the UV irradiated surface of the cloud to its cosmic-ray dominated centra