Zobrazeno 1 - 10
of 1 819
pro vyhledávání: '"Favre, C"'
Autor:
Lattanzi, V., Alves, F. O., Padovani, M., Fontani, F., Caselli, P., Ceccarelli, C., López-Sepulcre, A., Favre, C., Neri, R., Chahine, L., Vastel, C., Evans, L.
Publikováno v:
A&A 671, A35 (2023)
The study of the early phases of star and planet formation is important to understand the physical and chemical history of stellar systems such as our own. In particular, protostars born in rich clusters are prototypes of the young Solar System. In t
Externí odkaz:
http://arxiv.org/abs/2301.10267
Autor:
Chahine, L., López-Sepulcre, A., Podio, L., Codella, C., Neri, R., Mercimek, S., De Simone, M., Caselli, P., Ceccarelli, C., Bouvier, M., Sakai, N., Fontani, F., Yamamoto, S., Alves, F. O., Lattanzi, V., Evans, L., Favre, C.
Publikováno v:
A&A 667, A6 (2022)
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 are thought to split into collections of sonic fibres. The locations where
Externí odkaz:
http://arxiv.org/abs/2209.03696
Autor:
Ceccarelli, C., Codella, C., Balucani, N., Bockelée-Morvan, D., Herbst, E., Vastel, C., Caselli, P., Favre, C., Lefloch, B., Öberg, K.
Planetary systems such as our own are formed after a long process where matter condenses from diffuse clouds to stars, planets, asteroids, comets and residual dust, undergoing dramatic changes in physical and chemical state in less than a few million
Externí odkaz:
http://arxiv.org/abs/2206.13270
Autor:
Schutzer, A. de A., Rivera-Ortiz, P. R., Lefloch, B., Gusdorf, A., Favre, C., Segura-Cox, D., Lopez-Sepulcre, A., Neri, R., Ospina-Zamudio, J., De Simone, M., Codella, C., Viti, S., Podio, L., Pineda, J., O'Donoghue, R., Ceccarelli, C., Caselli, P., Alves, F., Bachiller, R., Balucani, N., Bianchi, E., Bizzocchi, L., Bottinelli, S., Caux, E., Chacón-Tanarro, A., Dulieu, F., Enrique-Romero, J., Fontani, F., Feng, S., Holdship, J., Jiménez-Serra, I., Al-Edhari, A. Jaber, Kahane, C., Lattanzi, V., Oya, Y., Punanova, A., Rimola, A., Sakai, N., Spezzano, S., Sims, I. R., Taquet, V., Testi, L., Theulé, P., Ugliengo, P., Vastel, C., Vasyunin, A. I., Vazart, F., Yamamoto, S., Witzel, A.
Publikováno v:
A&A 662, A104 (2022)
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 the nature of the driving so
Externí odkaz:
http://arxiv.org/abs/2203.09383
Autor:
Chahine, L., López-Sepulcre, A., Neri, R., Ceccarelli, C., Mercimek, S., Codella, C., Bouvier, M., Bianchi, E., Favre, C., Podio, L., Alves, F. O., Sakai, N., Yamamoto, S.
Publikováno v:
A&A 657, A78 (2022)
Hot corinos are compact regions around solar-mass protostellar objects that are very rich in interstellar complex organic molecules (iCOMs). They are believed to represent the very early phases of our Solar System's birth, which was very likely also
Externí odkaz:
http://arxiv.org/abs/2112.08077
Autor:
Codella, C., Bianchi, E., Podio, L., Mercimek, S., Ceccarelli, C., Lopez-Sepulcre, A., Bachiller, R., Caselli, P., Sakai, N., Neri, R., Fontani, F., Favre, C., Balucani, N., Lefloch, B., Viti, S., Yamamoto, S.
Publikováno v:
A&A 654, A52 (2021)
Aims: The goal is to obtain a census of S-bearing species using interferometric images, towards SVS13-A, a Class I object associated with a hot corino rich in interstellar complex organic molecules. Methods: We used data at 3mm and 1.4mm obtained wit
Externí odkaz:
http://arxiv.org/abs/2109.01142
Autor:
Codella, C., Podio, L., Garufi, A., Perrero, J., Ugliengo, P., Fedele, D., Favre, C., Bianchi, E., Ceccarelli, C., Mercimek, S., Bacciotti, F., Rygl, K. L. J., Testi, L.
Aims: To trace the radial and vertical spatial distribution of H2CS, a key species of the S-bearing chemistry, in protoplanetary disks. To analyse the observed distributions in light of the H2CS binding energy, in order to discuss the role of thermal
Externí odkaz:
http://arxiv.org/abs/2011.02305
Autor:
Podio, L., Garufi, A., Codella, C., Fedele, D., Rygl, K., Favre, C., Bacciotti, F., Bianchi, E., Ceccarelli, C., Mercimek, S., Teague, R., Testi, L.
Publikováno v:
A&A 644, A119 (2020)
Planets form in protoplanetary disks and inherit their chemical composition. It is therefore crucial to understand the disks molecular content. We aim to characterize the distribution and abundance of molecules in the disk of DG Tau. In the context o
Externí odkaz:
http://arxiv.org/abs/2011.01081
Autor:
Podio, L., Garufi, A., Codella, C., Fedele, D., Bianchi, E., Bacciotti, F., Ceccarelli, C., Favre, C., Mercimek, S., Rygl, K., Testi, L.
Publikováno v:
A&A 642, L7 (2020)
The chemical composition of planets is inherited from that of the protoplanetary disk at the time of planet formation. Increasing observational evidence suggests that planet formation occurs in less than 1 Myr. This motivates the need for spatially r
Externí odkaz:
http://arxiv.org/abs/2008.12648