Zobrazeno 1 - 10
of 302
pro vyhledávání: '"Zamudio J"'
Autor:
Vastel, C., Alves, F., Ceccarelli, C., Bouvier, M., Jimenez-Serra, I., Sakai, T., Caselli, P., Evans, L., Fontani, F., Gal, R. Le, Chandler, C. J., Svoboda, B., Maud, L., Codella, C., Sakai, N., Lopez-Sepulcre, A., Moellenbrock, G., Aikawa, Y., Balucani, N., Bianchi, E., Busquet, G., Caux, E., Charnley, S., Cuello, N., De Simone, M., Dulieu, F., Duran, A., Fedele, D., Feng, S., Francis, L., Hama, T., Hanawa, T., Herbst, E., Hirota, T., Imai, M., Isella, A., Johnstone, D., Lefloch, B., Loinard, L., Maureira, M., Murillo, N. M., Mercimek, S., Mori, S., Menard, F., Miotello, A., Nakatani, R., Nomura, H., Oba, Y., Ohashi, S., Okoda, Y., Ospina-Zamudio, J., Oya, Y., Pineda, J. E., Podio, L., Rimola, A., Cox, D. Segura, Shirley, Y., Testi, L., Viti, S., Watanabe, N., Watanabe, Y., Witzel, A., Xue, C., Zhang, Y., Zhao, B., Yamamoto, S.
Publikováno v:
A&A 664, A171 (2022)
Methanol is a ubiquitous species commonly found in the molecular interstellar medium. It is also a crucial seed species for the building-up of the chemical complexity in star forming regions. Thus, understanding how its abundance evolves during the s
Externí odkaz:
http://arxiv.org/abs/2206.10176
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:
Bianchi, E., Chandler, C. J., Ceccarelli, C., Codella, C., Sakai, N., López-Sepulcre, A., Maud, L. T., Moellenbrock, G., Svoboda, B., Watanabe, Y., Sakai, T., Ménard, F., Aikawa, Y., Alves, F., Balucani, N., Bouvier, M., Caselli, P., Caux, E., Charnley, S., Choudhury, S., De Simone, M., Dulieu, F., Durán, A., Evans, L., Favre, C., Fedele, D., Feng, S., Fontani, F., Francis, L., Hama, T., Hanawa, T., Herbst, E., Hirota, T., Imai, M., Isella, A., Jiménez-Serra, I., Johnstone, D., Kahane, C., Lefloch, B., Loinard, L., Maureira, M. J., Mercimek, S., Miotello, A., Mori, S., Nakatani, R., Nomura, H., Oba, Y., Ohashi, S., Okoda, Y., Ospina-Zamudio, J., Oya, Y., Pineda, J., Podio, L., Rimola, A., Cox, D. Segura, Shirley, Y., Taquet, V., Testi, L., Vastel, C., Viti, S., Watanabe, N., Witzel, A., Xue, C., Zhang, Y., Zhao, B., Yamamoto, S.
The study of hot corinos in Solar-like protostars has been so far mostly limited to the Class 0 phase, hampering our understanding of their origin and evolution. In addition, recent evidence suggests that planet formation starts already during Class
Externí odkaz:
http://arxiv.org/abs/2007.10275
Autor:
De Simone, M., Codella, C., Ceccarelli, C., López-Sepulcre, A., Witzel, A., Neri, R., Balucani, N., Caselli, P., Favre, C., Fontani, F., Lefloch, B., Ospina-Zamudio, J., Pineda, J. E., Taquet, V.
Publikováno v:
A&A 640, A75 (2020)
Aims: A unique environment to study how interstellar Complex Organic Molecules (iCOMs) can be formed is the shocked gas along low-mass protostellar outflows, as the dust mantles composition is sputtered into the gas phase. The chemical richness in th
Externí odkaz:
http://arxiv.org/abs/2006.09925
Autor:
Favre, C., Vastel, C., Jimenez-Serra, I., Quénard, D., Caselli, P., Ceccarelli, C., Chacón-Tanarro, A., Fontani, F., Holdship, J., Oya, Y., Punanova, A., Sakai, N., Spezzano, S., Yamamoto, S., Neri, R., López-Sepulcre, A., Alves, F., Bachiller, R., Balucani, N., Bianchi, E., Bizzocchi, L., Codella, C., Caux, E., De Simone, M., Romero, J. Enrique, Dulieu, F., Feng, S., Al-Edhari, A. Jaber, Lefloch, B., Ospina-Zamudio, J., Pineda, J., Podio, L., Rimola, A., Segura-Cox, D., Sims, I. R., Taquet, V., Testi, L., Theulé, P., Ugliengo, P., Vasyunin, A. I., Vazart, F., Viti, S., Witzel, A.
Publikováno v:
A&A 635, A189 (2020)
The SOLIS (Seeds Of Life In Space) IRAM/NOEMA Large Program aims at studying a set of crucial complex organic molecules in a sample of sources, with well-known physical structure, covering the various phases of Solar-type star formation. One represen
Externí odkaz:
http://arxiv.org/abs/2002.07004
Autor:
Ospina-Zamudio, J., Lefloch, B., Favre, C., López-Sepulcre, A., Bianchi, E., Ceccarelli, C., DeSimone, M., Bouvier, M., Kahane, C.
The chemical composition of protostellar jets and its origin are still badly understood. More observational constraints are needed to make progress. With that objective, we have carried out a systematic search for molecular species in the jet of Cep
Externí odkaz:
http://arxiv.org/abs/1909.12002
Akademický článek
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Autor:
Bianchi, E., Codella, C., Ceccarelli, C., Vazart, F., Bachiller, R., Balucani, N., Bouvier, M., De Simone, M., Enrique-Romero, J., Kahane, C., Lefloch, B., López-Sepulcre, A., Ospina-Zamudio, J., Podio, L., Taquet, V.
We present the first census of the interstellar Complex Organic Molecules (iCOMs) in the low-mass Class I protostar SVS13-A, obtained by analysing data from the IRAM-30m Large Project ASAI (Astrochemical Surveys At IRAM). They consist of an high-sens
Externí odkaz:
http://arxiv.org/abs/1810.11411
Autor:
Zamudio, J. Ospina, Lefloch, B., Ceccarelli, C., Kahane, C., Favre, C., López-Sepulcre, A., Montarges, M.
Publikováno v:
A&A 618, A145 (2018)
Intermediate-mass (IM) protostars provide a bridge between the low- and high-mass protostars. Despite their relevance, little is known about their chemical diversity. We want to investigate the molecular richness towards the envelope of IM protostars
Externí odkaz:
http://arxiv.org/abs/1807.11278
Autor:
Lefloch, B., Bachiller, R., Ceccarelli, C., Cernicharo, J., Codella, C., Fuente, A., Kahane, C., López-Sepulcre, A., Tafalla, M., Vastel, C., Caux, E., González-García, M., Bianchi, E., Gómez-Ruiz, A., Holdship, J., Mendoza, E., Ospina-Zamudio, J., Podio, L., Quénard, D., Roueff, E., Sakai, N., Viti, S., Yamamoto, S., Yoshida, K., Favre, C., Monfredini, T., Quitián-Lara, H. M., Marcelino, N., Boechat-Roberty, H. M., Cabrit, S.
Evidence is mounting that the small bodies of our Solar System, such as comets and asteroids, have at least partially inherited their chemical composition from the first phases of the Solar System formation. It then appears that the molecular complex
Externí odkaz:
http://arxiv.org/abs/1803.10292