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pro vyhledávání: '"M. Benedettini"'
Akademický článek
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Akademický článek
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Autor:
A Traficante, B M Jones, A Avison, G A Fuller, M Benedettini, D Elia, S Molinari, N Peretto, S Pezzuto, T Pillai, K L J Rygl, E Schisano, R J Smith
The formation mechanism of the most massive stars is far from completely understood. It is still unclear if the formation is core-fed or clump-fed, i.e. if the process is an extension of what happens in low-mass stars, or if the process is more dynam
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cc68713a46a69fc48f5bc63933341764
http://arxiv.org/abs/2301.09917
http://arxiv.org/abs/2301.09917
Akademický článek
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Akademický článek
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Autor:
E. Mendoza, Serena Viti, Linda Podio, Rafael Bachiller, P. R. Rivera-Ortiz, Bertrand Lefloch, Charlotte Vastel, M. Benedettini, Gemma Busquet, Jacques Raymond Daniel Lépine, C. Codella, A Schutzer
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Monthly Notices of the Royal Astronomical Society, 507(1), 1034-1046
Monthly Notices of the Royal Astronomical Society: Letters
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, In press
HAL
instname
Monthly Notices of the Royal Astronomical Society, 507(1), 1034-1046
Monthly Notices of the Royal Astronomical Society: Letters
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, In press
HAL
HCN and its isomer HNC play an important role in molecular cloud chemistry and the formation of more complex molecules. We investigate here the impact of protostellar shocks on the HCN and HNC abundances from high-sensitivity IRAM 30m observations of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::08ff3972ec38904904c7b3e3b085c13d
https://hdl.handle.net/1887/3264060
https://hdl.handle.net/1887/3264060
Autor:
R. Neri, C. Codella, M. Benedettini, Cecilia Ceccarelli, Linda Podio, Bertrand Lefloch, Gemma Busquet, Francesco Fontani, S. Viti, Charlotte Vastel, Ana López-Sepulcre, E. Bianchi, S. Spezzano, Paola Caselli
Publikováno v:
Astronomy & Astrophysics, 645, 1-7
The isotopic ratio of nitrogen presents a wide range of values in the Solar System and in star forming system whose origin is still unclear. Chemical reactions in the gas phase are one of the possible processes that could modify the $^{14}$N/$^{15}$N
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d7b7712108e2736fd46be16d2bcebf3
https://hdl.handle.net/1887/3256748
https://hdl.handle.net/1887/3256748
Autor:
M. T. Beltrán, K. L. J. Rygl, Alessio Traficante, Adriano Baldeschi, Luca Olmi, Jan Brand, Manuel Merello, S. J. Liu, M. Benedettini, Stefano Pezzuto, Eugenio Schisano, Francesco Fontani, Riccardo Cesaroni, Leonardo Testi, Sergio Molinari, Davide Elia
New-generation spectroscopic surveys of the Milky Way plane have been revealing the structure of the interstellar medium, allowing the simultaneous study of dense structures from single star-forming objects or systems to entire spiral arms. We presen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::458c897d60c358e9f9addf1d0a93defd
http://hdl.handle.net/20.500.12386/32469
http://hdl.handle.net/20.500.12386/32469
Autor:
Vera Konyves, E. Fiorellino, Stefano Pezzuto, M. Benedettini, Derek Ward-Thompson, Frédérique Motte, Ph. André, Andrea Bracco, J. Di Francesco, Doris Arzoumanian, Jason M. Kirk, Sylvain Bontemps, Eugenio Schisano, Sergio Molinari, Davide Elia, Alexander Men'shchikov
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2020, ⟨10.1093/mnras/staa3420⟩
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2020, ⟨10.1093/mnras/staa3420⟩
The Herschel Gould Belt survey mapped the nearby (d < 500 pc) star-forming regions to understand better how the prestellar phase influences the star formation process. Here we report a complete census of dense cores in a 15 deg2 area of the Serpens s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ebf8934c48830eaf6e5e1b3674d5e2a
http://arxiv.org/abs/2010.15241
http://arxiv.org/abs/2010.15241
Autor:
Stefano Pezzuto, Alexander Men'shchikov, Ph. André, J. Di Francesco, Christine D. Wilson, Sylvain Bontemps, L. Piccotti, Sarah Sadavoy, Frédérique Motte, Vera Konyves, P. Palmeirim, E. Fiorellino, Nicola Schneider, Jason M. Kirk, L. Spinoglio, Davide Elia, J.-Ph. Bernard, Eugenio Schisano, Doris Arzoumanian, G. Li Causi, M. Benedettini, Derek Ward-Thompson, Bilal Ladjelate
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 645, pp.A55. ⟨10.1051/0004-6361/201936534⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 645, pp.A55. ⟨10.1051/0004-6361/201936534⟩
(Abridged) In this paper, we present analyses of images taken with the Herschel ESA satellite from 70mu to 500mu. We first constructed column density and dust temperature maps. Next, we identified compact cores in the maps, and characterize the cores
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8b7f88d0a04cbebda5aaea7dbb59290b
http://arxiv.org/abs/2010.00006
http://arxiv.org/abs/2010.00006