Zobrazeno 1 - 10
of 346
pro vyhledávání: '"R. Bachiller"'
Autor:
A. de A. Schutzer, P. R. Rivera-Ortiz, B. Lefloch, A. Gusdorf, C. Favre, D. Segura-Cox, A. López-Sepulcre, R. Neri, J. Ospina-Zamudio, M. De Simone, C. Codella, S. Viti, L. Podio, J. Pineda, R. O’Donoghue, C. Ceccarelli, P. Caselli, F. Alves, R. Bachiller, N. Balucani, E. Bianchi, L. Bizzocchi, S. Bottinelli, E. Caux, A. Chacón-Tanarro, F. Dulieu, J. Enrique-Romero, F. Fontani, S. Feng, J. Holdship, I. Jiménez-Serra, A. Jaber Al-Edhari, C. Kahane, V. Lattanzi, Y. Oya, A. Punanova, A. Rimola, N. Sakai, S. Spezzano, I. R. Sims, V. Taquet, L. Testi, P. Theulé, P. Ugliengo, C. Vastel, A. I. Vasyunin, F. Vazart, S. Yamamoto, A. Witzel
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 662, pp.A104. ⟨10.1051/0004-6361/202142931⟩
Astronomy & Astrophysics, 662:A104
Astronomy and Astrophysics
Astronomy and Astrophysics-A&A, 2022, 662, pp.A104. ⟨10.1051/0004-6361/202142931⟩
Astronomy & Astrophysics, 662:A104
Astronomy and Astrophysics
Context. 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 on the nature of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cc7b401d29f97c3717cf6f67d916aa87
https://hdl.handle.net/11585/901234
https://hdl.handle.net/11585/901234
Akademický článek
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Autor:
A. Fuente, P. Rivière-Marichalar, L. Beitia-Antero, P. Caselli, V. Wakelam, G. Esplugues, M. Rodríguez-Baras, D. Navarro-Almaida, M. Gerin, C. Kramer, R. Bachiller, J. R. Goicoechea, I. Jiménez-Serra, J. C. Loison, A. Ivlev, R. Martín-Doménech, S. Spezzano, O. Roncero, G. Muñoz-Caro, S. Cazaux, N. Marcelino
Publikováno v:
Astronomy & Astrophysics, 670
Gas phase Elemental abundances in molecular CloudS (GEMS) is an IRAM 30m large program aimed at determining the elemental abundances of carbon (C), oxygen (O), nitrogen (N), and sulfur (S) in a selected set of prototypical star-forming filaments. In
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9947400133647893ac767164dc620d2f
We present sensitive $\rm NH_3$ (1,1)--(7,7) line images from the Karl G. Jansky Very Large Array toward successive shocks, which are associated with the blueshifted outflow lobe driven by the compact protobinary system L1157. Within a projection dis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7a6e8ee492f335cd09edde2dfc3fc7e5
Autor:
E. Bianchi, C. Ceccarelli, C. Codella, A. López-Sepulcre, S. Yamamoto, N. Balucani, P. Caselli, L. Podio, R. Neri, R. Bachiller, C. Favre, F. Fontani, B. Lefloch, N. Sakai, D. Segura-Cox
Publikováno v:
Astronomy & Astrophysics. 662:A103
Context. Deuteration is a precious tool for investigating the origin and formation routes of interstellar complex organic molecules in the different stages of the star formation process. Methyl cyanide (CH3CN) is one of the most abundant interstellar
Autor:
Patricia R. Bachiller, Amy E. Vinson
Publikováno v:
Paediatric anaesthesiaREFERENCES. 31(1)
Pediatric anesthesiologists practice within a culture, a system, and a society. In this article, we provide an overview of the influence these have on the well-being or the unwellness of pediatric anesthesiologists. The scope of these issues is broad
Autor:
C. Favre, C. Vastel, I. Jimenez-Serra, D. Quénard, P. Caselli, C. Ceccarelli, A. Chacón-Tanarro, F. Fontani, J. Holdship, Y. Oya, A. Punanova, N. Sakai, S. Spezzano, S. Yamamoto, R. Neri, A. López-Sepulcre, F. Alves, R. Bachiller, N. Balucani, E. Bianchi, L. Bizzocchi, C. Codella, E. Caux, M. De Simone, J. Enrique Romero, F. Dulieu, S. Feng, A. Jaber Al-Edhari, B. Lefloch, J. Ospina-Zamudio
Publikováno v:
Astronomy & Astrophysics
Autor:
V. Taquet, C. Codella, M. De Simone, A. López-Sepulcre, J. E. Pineda, D. Segura-Cox, C. Ceccarelli, P. Caselli, A. Gusdorf, M. V. Persson, F. Alves, E. Caux, C. Favre, F. Fontani, R. Neri, Y. Oya, N. Sakai, C. Vastel, S. Yamamoto, R. Bachiller, N. Balucani, E. Bianchi, L. Bizzocchi, A. Chacón-Tanarro, F. Dulieu, J. Enrique-Romero, S. Feng, J. Holdship, B. Lefloch, A. Jaber Al-Edhari, I. Jiménez-Serra, C. Kahane, V. Lattanzi, J. Ospina-Zamudio, L. Podio, A. Punanova, A. Rimola, I. R. Sims, S. Spezzano, L. Testi, P. Theulé, P. Ugliengo, A. I. Vasyunin, F. Vazart, S. Viti, A. Witzel
Publikováno v:
Astron. Astrophys.
Astronomy and Astrophysics
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 637, pp.A63. ⟨10.1051/0004-6361/201937072⟩
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A, 2020, 637, pp.A63. ⟨10.1051/0004-6361/201937072⟩
Universidad de Alicante (UA)
Astronomy and Astrophysics
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 637, pp.A63. ⟨10.1051/0004-6361/201937072⟩
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A, 2020, 637, pp.A63. ⟨10.1051/0004-6361/201937072⟩
Universidad de Alicante (UA)
Context. Low-mass protostars drive powerful molecular outflows that can be observed with millimetre and submillimetre telescopes. Various sulfuretted species are known to be bright in shocks and could be used to infer the physical and chemical condit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::07054e71d29db32d8f9a0132bb0275a6
https://hdl.handle.net/10995/101466
https://hdl.handle.net/10995/101466
Publikováno v:
Semergen. 46(2)
Autor:
A. Fuente, D. G. Navarro, P. Caselli, M. Gerin, C. Kramer, E. Roueff, T. Alonso-Albi, R. Bachiller, S. Cazaux, B. Commercon, R. Friesen, S. García-Burillo, B. M. Giuliano, J. R. Goicoechea, P. Gratier, A. Hacar, I. Jiménez-Serra, J. Kirk, V. Lattanzi, J. C. Loison, J. Malinen, N. Marcelino, R. Martín-Doménech, G. Muñoz-Caro, J. Pineda, M. Tafalla, B. Tercero, D. Ward-Thompson, S. P. Treviño
Publikováno v:
Astronomy & Astrophysics