Zobrazeno 1 - 10
of 1 680
pro vyhledávání: '"M. DE SIMONE"'
Autor:
L. Cacciapuoti, L. Testi, L. Podio, C. Codella, A. J. Maury, M. De Simone, P. Hennebelle, U. Lebreuilly, R. S. Klessen, S. Molinari
Publikováno v:
The Astrophysical Journal, Vol 961, Iss 1, p 90 (2024)
Low dust opacity spectral indices ( β < 1) measured in the inner envelopes of class 0/I young stellar objects (age ∼10 ^4–5 yr) have been interpreted as the presence of (sub-)millimeter dust grains in these environments. The density conditions a
Externí odkaz:
https://doaj.org/article/f2f1f79b974a4b05a83659b516c8ea6c
Autor:
M. Villenave, L. Podio, G. Duchêne, K. R. Stapelfeldt, C. Melis, C. Carrasco-Gonzalez, V. J. M. Le Gouellec, F. Ménard, M. de Simone, C. Chandler, A. Garufi, C. Pinte, E. Bianchi, C. Codella
Publikováno v:
The Astrophysical Journal, Vol 946, Iss 2, p 70 (2023)
We present new Very Large Array observations, between 6.8 and 66 mm, of the edge-on Class I disk IRAS04302+2247. Observations at 6.8 mm and 9.2 mm lead to the detection of thermal emission from the disk, while shallow observations at the other wavele
Externí odkaz:
https://doaj.org/article/27f9952f3ad94f6f93b35659dd0ae671
Autor:
S Mercimek, L Podio, C Codella, L Chahine, A López-Sepulcre, S Ohashi, L Loinard, D Johnstone, F Menard, N Cuello, P Caselli, J Zamponi, Y Aikawa, E Bianchi, G Busquet, J E Pineda, M Bouvier, M De Simone, Y Zhang, N Sakai, C J Chandler, C Ceccarelli, F Alves, A Durán, D Fedele, N Murillo, I Jiménez-Serra, S Yamamoto
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 522:2384-2392
More than 50% of solar-mass stars form in multiple systems. It is therefore crucial to investigate how multiplicity affects the star and planet formation processes at the protostellar stage. We report continuum and C$^{18}$O (2-1) observations of the
Akademický článek
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Publikováno v:
PCCP. Physical chemistry chemical physics
24 (2022): 1993–2003. doi:10.1039/d1cp05264k
info:cnr-pdr/source/autori:Totani R.; Ljubic I.; Ciavardini A.; Grazioli C.; Galdenzi F.; De Simone M.; Coreno M./titolo:Frontier orbital stability of nitroxyl organic radicals probed by means of inner shell resonantly enhanced valence band photoelectron spectroscopy/doi:10.1039%2Fd1cp05264k/rivista:PCCP. Physical chemistry chemical physics (Print)/anno:2022/pagina_da:1993/pagina_a:2003/intervallo_pagine:1993–2003/volume:24
24 (2022): 1993–2003. doi:10.1039/d1cp05264k
info:cnr-pdr/source/autori:Totani R.; Ljubic I.; Ciavardini A.; Grazioli C.; Galdenzi F.; De Simone M.; Coreno M./titolo:Frontier orbital stability of nitroxyl organic radicals probed by means of inner shell resonantly enhanced valence band photoelectron spectroscopy/doi:10.1039%2Fd1cp05264k/rivista:PCCP. Physical chemistry chemical physics (Print)/anno:2022/pagina_da:1993/pagina_a:2003/intervallo_pagine:1993–2003/volume:24
We have investigated the frontier orbitals of persistent organic radicals known as nitroxyls by resonant photoelectron spectroscopy (ResPES) under inner shell excitation. By means of this site-specific technique, we were able to disentangle the diffe
Publikováno v:
ICERI2022 Proceedings.
Autor:
L. Chahine, A. López-Sepulcre, L. Podio, C. Codella, R. Neri, S. Mercimek, M. De Simone, P. Caselli, C. Ceccarelli, M. Bouvier, N. Sakai, F. Fontani, S. Yamamoto, F. O. Alves, V. Lattanzi, L. Evans, C. Favre
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 667, ⟨10.1051/0004-6361/202243799⟩
Astronomy and Astrophysics-A&A, 2022, 667, ⟨10.1051/0004-6361/202243799⟩
Context. Star-forming molecular clouds are characterised by the ubiquity of intertwined filaments. The filaments have been observed in both high- and low-mass star-forming regions, and they are thought to split into collections of sonic fibres. The l
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::24a308899c6c8c332742adaa1238473a
http://arxiv.org/abs/2209.03696
http://arxiv.org/abs/2209.03696
Autor:
A. de A. Schutzer, P. R. Rivera-Ortiz, B. Lefloch, A. Gusdorf, C. Favre, D. Segura-Cox, A. López-Sepulcre, R. Neri, J. Ospina-Zamudio, M. De Simone, C. Codella, S. Viti, L. Podio, J. Pineda, R. O’Donoghue, C. Ceccarelli, P. Caselli, F. Alves, R. Bachiller, N. Balucani, E. Bianchi, L. Bizzocchi, S. Bottinelli, E. Caux, A. Chacón-Tanarro, F. Dulieu, J. Enrique-Romero, F. Fontani, S. Feng, J. Holdship, I. Jiménez-Serra, A. Jaber Al-Edhari, C. Kahane, V. Lattanzi, Y. Oya, A. Punanova, A. Rimola, N. Sakai, S. Spezzano, I. R. Sims, V. Taquet, L. Testi, P. Theulé, P. Ugliengo, C. Vastel, A. I. Vasyunin, F. Vazart, S. Yamamoto, A. Witzel
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 662, pp.A104. ⟨10.1051/0004-6361/202142931⟩
Astronomy & Astrophysics, 662:A104
Astronomy and Astrophysics
Astronomy and Astrophysics-A&A, 2022, 662, pp.A104. ⟨10.1051/0004-6361/202142931⟩
Astronomy & Astrophysics, 662:A104
Astronomy and Astrophysics
Context. Protostellar jets are an important agent of star formation feedback, tightly connected with the mass-accretion process. The history of jet formation and mass ejection provides constraints on the mass accretion history and on the nature of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cc7b401d29f97c3717cf6f67d916aa87
https://hdl.handle.net/11585/901234
https://hdl.handle.net/11585/901234