Zobrazeno 1 - 10
of 127
pro vyhledávání: '"Muñoz-Caro G"'
Autor:
Fuente, A., Rivière-Marichalar, P., Beitia-Antero, L., Caselli, P., Wakelam, V., Esplugues, G., Rodríguez-Baras, M., Navarro-Almaida, D., Gerin, M., Kramer, C., Bachiller, R., Goicoechea, J. R., Jiménez-Serra, I., Loison, J. C., Ivlev, A., Martín-Doménech, R., Spezzano, S., Roncero, O., Muñoz-Caro, G., Cazaux, S., Marcelino, N.
Publikováno v:
A&A 670, A114 (2023)
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:
http://arxiv.org/abs/2212.03742
Autor:
Rodríguez-Baras, M., Fuente, A., Riviére-Marichalar, P., Navarro-Almaida, D., Caselli, P., Gerin, M., Kramer, C., Roueff, E., Wakelam, V., Esplugues, G., García-Burillo, S., Gal, R. Le, Spezzano, S., Alonso-Albi, T., Bachiller, R., Cazaux, S., Commercon, B., Goicoechea, J. R., Loison, J. C., Treviño-Morales, S. P., Roncero, O., Jiménez-Serra, I., Laas, J., Hacar, A., Kirk, J., Lattanzi, V., Martín-Doménech, R., Muñoz-Caro, G., Pineda, J. E., Tercero, B., Ward-Thompson, D., Tafalla, M., Marcelino, N., Malinen, J., Friesen, R., Giuliano, B. M.
Publikováno v:
A&A 648, A120 (2021)
Gas phase Elemental abundances in Molecular CloudS (GEMS) is an IRAM 30m Large Program designed to estimate the S, C, N, and O depletions and gas ionization degree, X(e-), in a set of star-forming filaments of Taurus, Perseus and Orion. Our immediate
Externí odkaz:
http://arxiv.org/abs/2102.13153
Autor:
Bulut, N., Roncero, O., Aguado, A., Loison, J. -C., Navarro-Almaida, D., Wakelam, V., Fuente, A., Roueff, E., Gal, R. Le, Caselli, P., Hickson, M. Gerinm K. M., Spezzano, S., Riviere-Marichalar, P., Alonso-Albi, T., Bachiller, R., Jimenez-Serra, I., Kramer, C., Tercero, B., Rodriguez-Baras, M., Garcia-Burillo, S., Goicoechea, J. R., Treviño-Morales, S. P., Esplugues, G., Cazaux, S., Commercon, B., Laas, J., Kirk, J., Lattanzi, V., Martin-Domenech, R., Muñoz-Caro, G., Pineda, J., Ward-Thompson, D., Tafalla, M., Marcelino, N., Malinen, J., Friesen, R., Giuliano, B. M., Agundez, M., Hacar, A.
Publikováno v:
Astronomy & Astrophysics 646, A5 (2021)
CS is among the most abundant gas-phase S-bearing molecules in cold dark molecular clouds. It is easily observable with several transitions in the millimeter wavelength range, and has been widely used as a tracer of the gas density in the interstella
Externí odkaz:
http://arxiv.org/abs/2012.10176
Autor:
Fuente, A., Navarro, D., Caselli, P., Gerin, M., Kramer, C., Roueff, E., Alonso-Albi, T., Bachiller, R., Cazaux, S., Commercon, B., Friesen, R., García-Burillo, S., Giuliano, B. M., Goicoechea, J. R., Gratier, P., Hacar, A., Jiménez-Serra, I., Kirk, J., Lattanzi, V., Loison, J. C., Malinen, P. J., Marcelino, N., Martín-Doménech, R., Muñoz-Caro, G., Pineda, J., Tafalla, M., Tercero, B., Ward-Thompson, D., Treviño-Morales, S., Riviére-Marichalar, P., Roncero, O., Vidal, T., Ballester, Maikel Y.
GEMS is an IRAM 30m Large Program whose aim is determining the elemental depletions and the ionization fraction in a set of prototypical star-forming regions. This paper presents the first results from the prototypical dark cloud TMC 1. Extensive mil
Externí odkaz:
http://arxiv.org/abs/1809.04978
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Sep2024, Vol. 533 Issue 1, p967-978, 12p
Publikováno v:
Astron.Astrophys. 423 (2004) 549-558
We present ESO - Very Large Telescope and ESA - Infrared Space Observatory 3 to 4 $\mu$m spectra of Seyfert 2 nuclei as compared to our galactic center lines of sight. The diffuse interstellar medium probed in both environments displays the character
Externí odkaz:
http://arxiv.org/abs/astro-ph/0405327
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 10/20/2023, Vol. 525 Issue 2, p2690-2700, 11p
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Akademický článek
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Autor:
Cazaux, S.M., Carrascosa, H., Muñoz Caro, G. M., Caselli, P., Fuente, A., Navarro-Almaida, D., Riviére-Marichalar, P.
Publikováno v:
Astronomy & Astrophysics, 657
Context. Sulfur is a biogenic element used as a tracer of the evolution of interstellar clouds to stellar systems. However, most of the expected sulfur in molecular clouds remains undetected. Sulfur disappears from the gas phase in two steps. The fir
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::c72abcd372a539a4da20fb5ab1d7e6bb
http://resolver.tudelft.nl/uuid:4c554dce-7ba9-4e6b-a02d-48a70f20c224
http://resolver.tudelft.nl/uuid:4c554dce-7ba9-4e6b-a02d-48a70f20c224