Zobrazeno 1 - 10
of 8 848
pro vyhledávání: '"M de Simone"'
Publikováno v:
Il Foro Italiano, 1957 Jan 01. 80, 235/236-239/240.
Externí odkaz:
https://www.jstor.org/stable/23149378
Publikováno v:
Il Foro Italiano, 1956 Jan 01. 79, 137/138-141/142.
Externí odkaz:
https://www.jstor.org/stable/23146363
Publikováno v:
Il Foro Italiano, 1914 Jan 01. 39, 193/194-199/200.
Externí odkaz:
https://www.jstor.org/stable/23115132
Autor:
Zarmakoupi, Mantha
Publikováno v:
The Journal of Roman Studies, 2010 Jan 01. 100, 331-332.
Externí odkaz:
https://www.jstor.org/stable/41724845
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:
Mantha Zarmakoupi
Publikováno v:
Journal of Roman Studies. 100:331-332
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::40e59d07ed4ccb780e9fadc9a69047df
https://doi.org/10.1017/s0075435810000882
https://doi.org/10.1017/s0075435810000882
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fbdacc70fdabe465e32e387c8a39d6b3
https://doi.org/10.1093/mnras/stad964
https://doi.org/10.1093/mnras/stad964
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