Zobrazeno 1 - 10
of 64
pro vyhledávání: '"J R, Goicoechea"'
Autor:
Pierre Palud, Pierre Chainais, Franck Le Petit, Emeric Bron, Pierre-Antoine Thouvenin, Maxime Vono, L. Einig, M. Garcia Santa-Maria, M. Gaudel, J. H. Orkisz, V. de Souza Magalhaes, S. Bardeau, M. Gerin, J. R. Goicoechea, P. Gratier, V. V. Guzman, J. Kainulainen, F. Levrier, N. Peretto, J. Pety, A. Roueff, A. Sievers
Publikováno v:
2022 30th European Signal Processing Conference (EUSIPCO).
Autor:
Ü. Kavak, J. Bally, J. R. Goicoechea, C. H. M. Pabst, F. F. S. van der Tak, A. G. G. M. Tielens
Publikováno v:
Astronomy & Astrophysics, 663:A117
Astronomy and astrophysics, 663:A117. EDP Sciences
Astronomy and astrophysics, 663:A117. EDP Sciences
17 pags., 18 figs., 3 tabs.
Context. Interest in stellar feedback has recently increased because new studies suggest that radiative and mechanical feedback from young massive stars significantly regulates the physical and chemical composition of
Context. Interest in stellar feedback has recently increased because new studies suggest that radiative and mechanical feedback from young massive stars significantly regulates the physical and chemical composition of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d5ae315d925abe68ac71001355f8bc9d
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
Autor:
Ü. Kavak, J. R. Goicoechea, C. H. M. Pabst, J. Bally, F. F. S. van der Tak, A. G. G. M. Tielens
Publikováno v:
Astronomy and astrophysics, 660:A109. EDP Sciences
Astronomy & Astrophysics, 660:A109
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & Astrophysics, 660:A109
Digital.CSIC. Repositorio Institucional del CSIC
instname
20 pags., 20 figs., 2 tabs.
Context. The role of feedback in the self-regulation of star formation is a fundamental question in astrophysics. The Orion Nebula is the nearest site of ongoing and recent massive star formation. It is a unique labor
Context. The role of feedback in the self-regulation of star formation is a fundamental question in astrophysics. The Orion Nebula is the nearest site of ongoing and recent massive star formation. It is a unique labor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7205eacf8df3b7ee7438c29c2a8e4439
https://doi.org/10.1051/0004-6361/202141367
https://doi.org/10.1051/0004-6361/202141367
Autor:
R. Güsten, S. Kabanovic, Ronan Higgins, Mark G. Wolfire, O. Berne, Aggm Tielens, J. R. Goicoechea, D. Teyssier, C. H. M. Pabst, J. Stutzki, E. Chambers, C. Kramer, Alvaro Hacar
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 658, ⟨10.1051/0004-6361/202140805⟩
Astronomy & Astrophysics, 658:A98
Astronomy and Astrophysics-A&A, 2022, 658, ⟨10.1051/0004-6361/202140805⟩
Astronomy & Astrophysics, 658:A98
34 pags., 34 figs., 15 tabs.
Context. The [C II] 158 m fine-structure line is the dominant cooling line of moderate-density photodissociation regions (PDRs) illuminated by moderately bright far-ultraviolet (FUV) radiation fields. This makes this
Context. The [C II] 158 m fine-structure line is the dominant cooling line of moderate-density photodissociation regions (PDRs) illuminated by moderately bright far-ultraviolet (FUV) radiation fields. This makes this
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::224e8b905da3c9f07c8dd3fea477f55a
https://hal-insu.archives-ouvertes.fr/insu-03672056/file/aa40805-21.pdf
https://hal-insu.archives-ouvertes.fr/insu-03672056/file/aa40805-21.pdf
Autor:
J. R. Goicoechea, E. Verdasco, Pablo G. Jambrina, Alexander Zanchet, F. J. Aoiz, Marcelino Agúndez, M. Menéndez, A. Veselinova
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astron Astrophys
instname
Astron Astrophys
13 pags., 3 figs., 1 tab.
The reaction between atomic oxygen and molecular hydrogen is an important one in astrochemistry as it regulates the abundance of the hydroxyl radical and serves to open the chemistry of oxygen in diverse astronomical en
The reaction between atomic oxygen and molecular hydrogen is an important one in astrochemistry as it regulates the abundance of the hydroxyl radical and serves to open the chemistry of oxygen in diverse astronomical en
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5ae7a8d07910785d67e2f82785077a02
http://hdl.handle.net/10261/257940
http://hdl.handle.net/10261/257940
Autor:
Charles M. Bradford, Klaus M. Pontoppidan, Quentin Kral, Agata Karska, Maryvonne Gerin, Stefanie N. Milam, Jean-Michel Desert, Michiel R. Hogerheijde, Matthew Joseph Griffin, Asantha Cooray, D. W. Pesce, T. L. Roellig, Jayne Birkby, Itsuki Sakon, Susanne Aalto, Chris Pearson, E. A. Bergin, Denis Burgarella, G. Melnick, Paola Caselli, Vassilis Charmandaris, David Leisawitz, Mikako Matsuura, Paul Hartogh, L. K. Hunt, Frank Helmich, Lee Armus, E. De Beck, Johannes G. Staguhn, J. R. Goicoechea, Dimitra Rigopoulou, Kevin B. Stevenson, Margaret Meixner, A. Pope, Martina C. Wiedner
Publikováno v:
Experimental Astronomy, 51(3), 595-624. SPRINGER
Experimental Astronomy, 51(3), 595-624. Springer Netherlands
Exper.Astron.
Exper.Astron., 2021, 51 (3), pp.595-624. ⟨10.1007/s10686-021-09782-0⟩
Experimental Astronomy, 51(3), 595-624
Experimental Astronomy
Experimental Astronomy, 51(3), 595-624. Springer Netherlands
Exper.Astron.
Exper.Astron., 2021, 51 (3), pp.595-624. ⟨10.1007/s10686-021-09782-0⟩
Experimental Astronomy, 51(3), 595-624
Experimental Astronomy
The Origins Space Telescope (Origins) is one of four science and technology definition studies selected by the National Aeronautics and Space Administration (NASA) in preparation of the 2020 Astronomy and Astrophysics Decadal survey in the US. Origin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::873dd10f18ebb7d778057a67c03a01cf
https://hdl.handle.net/1887/3275476
https://hdl.handle.net/1887/3275476
Autor:
Jacob C. Laas, C. Kramer, Rachel Friesen, Benoît Commerçon, Mario Tafalla, Niyazi Bulut, T. Alonso-Albi, Kevin M. Hickson, Valerio Lattanzi, S. Spezzano, Paola Caselli, Rafael Bachiller, Jaime E. Pineda, Johanna Malinen, Octavio Roncero, G. Muñoz-Caro, R. Martin-Domenech, E. Roueff, Alfredo Aguado, R. Le Gal, G. B. Esplugues, Pablo Riviere-Marichalar, Barbara M. Giuliano, Alvaro Hacar, Belén Tercero, Jason M. Kirk, A. Fuente, Santiago García-Burillo, Jean-Christophe Loison, Derek Ward-Thompson, Nuria Marcelino, Valentine Wakelam, Izaskun Jiménez-Serra, Maryvonne Gerin, Marcelino Agúndez, M. Rodríguez-Baras, S. P. Treviño-Morales, J. R. Goicoechea, D. Navarro-Almaida, Stéphanie Cazaux
Publikováno v:
Astronomy and Astrophysics, 646
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 646, pp.A5. ⟨10.1051/0004-6361/202039611⟩
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Universitat Pompeu Fabra
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 646, pp.A5. ⟨10.1051/0004-6361/202039611⟩
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Universitat Pompeu Fabra
Artículo escrito por un elevado número de autores, solo se referencia el que aparece en primer lugar, el nombre del grupo de colaboración, si lo hubiere, y los autores pertenecientes a la UAM
Context. Carbon monosulphide (CS) is among the mos
Context. Carbon monosulphide (CS) is among the mos
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::50fa2ca8b26374c06ed8499204ce289e
http://hdl.handle.net/1887/3270741
http://hdl.handle.net/1887/3270741
Autor:
S. P. Treviño-Morales, J. R. Goicoechea, Mario Tafalla, T. Alonso-Albi, Barbara M. Giuliano, Valerio Lattanzi, Paola Caselli, Rafael Martín-Doménech, Belén Tercero, R. Le Gal, Jaime E. Pineda, D. Navarro-Almaida, Stéphanie Cazaux, Pablo Riviere-Marichalar, Jean-Christophe Loison, C. Kramer, Benoît Commerçon, Rafael Bachiller, G. M. Muñoz Caro, Jacob C. Laas, Nuria Marcelino, Maryvonne Gerin, Jason M. Kirk, Rachel Friesen, Santiago García-Burillo, Alvaro Hacar, Derek Ward-Thompson, Johanna Malinen, Valentine Wakelam, Octavio Roncero, E. Roueff, Izaskun Jiménez-Serra, A. Fuente
Publikováno v:
Astron Astrophys
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy & Astrophysics, 637, A39
instname
Digital.CSIC. Repositorio Institucional del CSIC
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy & Astrophysics, 637, A39
instname
Digital.CSIC. Repositorio Institucional del CSIC
21 pags., 16 figs., 7 tabs., 2 apps.
Context. Sulphur is one of the most abundant elements in the Universe. Surprisingly, sulphuretted molecules are not as abundant as expected in the interstellar medium and the identity of the main sulphur rese
Context. Sulphur is one of the most abundant elements in the Universe. Surprisingly, sulphuretted molecules are not as abundant as expected in the interstellar medium and the identity of the main sulphur rese
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::77855a5a82a179e4855dfe35639cd283
https://europepmc.org/articles/PMC7305024/
https://europepmc.org/articles/PMC7305024/
Publikováno v:
Astronomy and astrophysics. 616
The properties of molecular gas, the fuel that forms stars, inside the cavity of the circumnuclear disk (CND) are not well constrained. We present results of a velocity-resolved submillimeter scan (~480 to 1250 GHz) and [C ii] 158 μm line observatio