Zobrazeno 1 - 10
of 1 270
pro vyhledávání: '"C. Ceccarelli"'
Publikováno v:
AIP Advances, Vol 14, Iss 3, Pp 035109-035109-10 (2024)
The formation of CN and its isotopologue C15N through radiative association has been investigated. We considered two processes for the collisions of ground state C(3P) and N(4S) atoms (A2Π → X2Σ+ and b4Π → a4Σ+), as well as, for the first tim
Externí odkaz:
https://doaj.org/article/ad0b2ae069534b8991155c55e8a6630d
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 8 (2021)
The huge variety of planetary systems discovered in recent decades likely depends on the early history of their formation. In this contribution, we introduce the FAUST Large Program which focuses specifically on the early history of solar-like protos
Externí odkaz:
https://doaj.org/article/95d7e2a232304aed8d9a653068ff9bc1
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
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
C. Ceccarelli, E. Prina, O. Muneghina, M. Jordans, E. Barker, K. Miller, R. Singh, C. Acarturk, K. Sorsdhal, P. Cuijpers, C. Lund, C. Barbui, M. Purgato
Publikováno v:
Epidemiology and Psychiatric Sciences, 31:e75. Cambridge University Press
Epidemiology and Psychiatric Sciences, 31:e75, 1-7. Cambridge University Press
Ceccarelli, C, Prina, E, Muneghina, O, Jordans, M, Barker, E, Miller, K, Singh, R, Acarturk, C, Sorsdhal, K, Cuijpers, P, Lund, C, Barbui, C & Purgato, M 2022, ' Adverse childhood experiences and global mental health : avenues to reduce the burden of child and adolescent mental disorders ', Epidemiology and Psychiatric Sciences, vol. 31, e75, pp. 1-7 . https://doi.org/10.1017/S2045796022000580
Epidemiology and Psychiatric Sciences, 31:e75, 1-7. Cambridge University Press
Ceccarelli, C, Prina, E, Muneghina, O, Jordans, M, Barker, E, Miller, K, Singh, R, Acarturk, C, Sorsdhal, K, Cuijpers, P, Lund, C, Barbui, C & Purgato, M 2022, ' Adverse childhood experiences and global mental health : avenues to reduce the burden of child and adolescent mental disorders ', Epidemiology and Psychiatric Sciences, vol. 31, e75, pp. 1-7 . https://doi.org/10.1017/S2045796022000580
Mental disorders are one of the largest contributors to the burden of disease globally, this holds also for children and adolescents, especially in low- and middle-income countries. The prevalence and severity of these disorders are influenced by soc
Autor:
A. Remijan, C. Xue, L. Margulès, A. Belloche, R. A. Motiyenko, J. Carder, C. Codella, N. Balucani, C. L. Brogan, C. Ceccarelli, T. R. Hunter, A. Maris, S. Melandri, M. Siebert, B. A. McGuire
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 658, ⟨10.1051/0004-6361/202142504⟩
Astronomy and Astrophysics-A&A, 2022, 658, ⟨10.1051/0004-6361/202142504⟩
Thioacetamide (CH3CSNH2) is the sulfur analog to acetamide (CH3CONH2) and it is a viable candidate to search for in astronomical environments specifically toward regions where other S-bearing molecules have been found and, if possible, that also cont
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d82fe906bea5d60cdf851dd26ee75f23
https://hal.science/hal-03660669/document
https://hal.science/hal-03660669/document
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