Zobrazeno 1 - 3
of 3
pro vyhledávání: '"J. D. Martin Ramos"'
Autor:
S. Direito, I. Fleischer, Nicolas Walter, Felipe Gómez, J. Kviderova, David Blake, Miriam García-Villadangos, A.K. Klingelhofer, J. D. Martin Ramos, Alberto Behar, P. Mahapatra, Victor Parro, Ricardo Amils, Philippe Sarrazin, Christina N. Stam, Kasthuri Venkateswaran, Mary A. Voytek, B.H. Foing, Fernando Rull
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
International Journal of Astrobiology, 10 (3), 2011
Gomez, F, Walter, N, Amils, R, Rull, F, Klingelhofer, A K, Kviderova, J, Sarrazin, P, Foing, B H, Behar, A, Fleischer, I, Parro, V, Garcia-Villadangos, M, Blake, D, Martin Ramos, J D, Direito, S, Mahapatra, P, Stam, C, Venkateswaran, K & Voytek, M 2011, ' Multidisciplinary integrated field campaign to an acidic Martian Earth analogue with astrobiological interest: Rio Tinto ', International Journal of Astrobiology, vol. 10, no. 10, 3, pp. 291-305 . https://doi.org/10.1017/S147355041100005X
International Journal of Astrobiology, 10(10):3, 291-305. Cambridge University Press
instname
International Journal of Astrobiology, 10 (3), 2011
Gomez, F, Walter, N, Amils, R, Rull, F, Klingelhofer, A K, Kviderova, J, Sarrazin, P, Foing, B H, Behar, A, Fleischer, I, Parro, V, Garcia-Villadangos, M, Blake, D, Martin Ramos, J D, Direito, S, Mahapatra, P, Stam, C, Venkateswaran, K & Voytek, M 2011, ' Multidisciplinary integrated field campaign to an acidic Martian Earth analogue with astrobiological interest: Rio Tinto ', International Journal of Astrobiology, vol. 10, no. 10, 3, pp. 291-305 . https://doi.org/10.1017/S147355041100005X
International Journal of Astrobiology, 10(10):3, 291-305. Cambridge University Press
Recently reported results from latest Mars Orbiters and Rovers missions are transforming our opinion about the red planet. That dry and inhospitable planet reported in the past is becoming a wetter planet with high probabilities of water existence in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::333d84f3b3be000acea59ef8a9ea193c
http://hdl.handle.net/10261/57826
http://hdl.handle.net/10261/57826
Autor:
J. D. Martin-Ramos, J. Molina Molina, J. F. Rodriguez Amo, A. B. Martinez-Aragon, J. A. Lopez Sastre, X. Solans
Publikováno v:
ChemInform. 24
Publikováno v:
Acta Crystallographica Section C Crystal Structure Communications. 48:957-959
C 11 H 11 N 3 O 2 cristallise dans P2 1 /c avec a=9.009, b=7.882, c=15.072A, β=98.61°, Z+4; affinement jusqu'a R=0.046. La structure est constituee d'empilements d'oximes. L'angle entre les groupes phenyl et imidazole est de 43.3°. Les deviations