Ciaravella, A., Osservatorio Astronomico di Palermo, Istituto Nazionale di Astrofisica, Palermo, 90134, Italy; Muñoz Caro, G.M., Centro de Astrobiología, Consejo Superior de Investigaciones Científicas, Instituto Nacional de Técnica Aeroespacial, Torrejón de Ardoz, Madrid, 28850, Spain; Jiménez-Escobar, A., Osservatorio Astronomico di Palermo, Istituto Nazionale di Astrofisica, Palermo, 90134, Italy; Cecchi-Pestellini, C., Osservatorio Astronomico di Palermo, Istituto Nazionale di Astrofisica, Palermo, 90134, Italy; Hsiao, L.-C., Department of Physics, National Central University, Jhongli, 32054, Taiwan; Huang, C.-H., Department of Physics, National Central University, Jhongli, 32054, Taiwan; Chen, Y.-J., Department of Physics, National Central University, Jhongli, 32054, Taiwan
Recommended Citation:
Ciaravella A.,Muñoz Caro G.M.,Jiménez-Escobar A.,et al. X-ray processing of a realistic ice mantle can explain the gas abundances in protoplanetary disks[J]. Proceedings of the National Academy of Sciences of the United States of America,2020-01-01,117(28)