Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Thomas Nony"'
Autor:
Roberto Galván-Madrid, Daniel J. Díaz-González, Frédérique Motte, Adam Ginsburg, Nichol Cunningham, Karl M. Menten, Mélanie Armante, Mélisse Bonfand, Jonathan Braine, Timea Csengeri, Pierre Dell’Ova, Fabien Louvet, Thomas Nony, Rudy Rivera-Soto, Patricio Sanhueza, Amelia M. Stutz, Friedrich Wyrowski, Rodrigo H. Álvarez-Gutiérrez, Tapas Baug, Sylvain Bontemps, Leonardo Bronfman, Manuel Fernández-López, Antoine Gusdorf, Atanu Koley, Hong-Li Liu, Javiera Salinas, Allison P. M. Towner, Anthony P. Whitworth
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 274, Iss 1, p 15 (2024)
We use the H41 α recombination line to create templates of the millimeter free–free emission in the ALMA-IMF continuum maps, which allows us to separate it from dust emission. This method complements spectral-index information and extrapolation fr
Externí odkaz:
https://doaj.org/article/0b10ed6f258143538914748f231323c6
Autor:
Daniel J. Díaz-González, Roberto Galván-Madrid, Adam Ginsburg, Frédérique Motte, Pierre Dell’Ova, Stanley Kurtz, Nichol Cunningham, Amelia M. Stutz, Fabien Louvet, Timea Csengeri, Manuel Fernández-López, Patricio Sanhueza, Thomas Nony, Rudy Rivera-Soto, Rodrigo H. Álvarez-Gutiérrez, Melanie Armante, Melisse Bonfand, Sylvain Bontemps, Antoine Gusdorf, Hong-Li Liu
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 269, Iss 2, p 55 (2023)
We present the combination of ALMA-IMF and single-dish continuum images from the MUSTANG-2 Galactic Plane Survey (MGPS90) at 3 mm and the Bolocam Galactic Plane Survey (BGPS) at 1 mm. Six and 10 out of the 15 ALMA-IMF fields are combined with MGPS90
Externí odkaz:
https://doaj.org/article/d50354177f4345d589a5704927e4fbec
Autor:
Patrick Hennebelle, Ugo Lebreuilly, Tine Colman, Davide Elia, Gary Fuller, Silvia Leurini, Thomas Nony, Eugenio Schisano, Juan D. Soler, Alessio Traficante, Ralf S. Klessen, Sergio Molinari, Leonardo Testi
Publikováno v:
Astronomy & Astrophysics. 668:A147
Context. In spite of decades of theoretical efforts, the physical origin of the stellar initial mass function (IMF) is still a subject of debate. Aims. We aim to gain an understanding of the influence of various physical processes such as radiative s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6fc82587134cd92af54b01824c3324e5
https://doi.org/10.1051/0004-6361/202243803
https://doi.org/10.1051/0004-6361/202243803