Differences

This shows you the differences between two versions of the page.

--- molecules:ism:ch3-plus [2025/12/30 11:15] – mueller
+++ molecules:ism:ch3-plus [2025/12/30 11:42] (current) – mueller
@@ Line 10: / Line 10: @@
 A much better modeling of the observed spectrum was achieved later by\\
 P. B. Changala, N. L. Chen, H. L. Le, B. Gans, K. Steenbakkers, T. Salomon, L. Bonah, I. Schroetter, A. Canin, M.-A. Martin-Drumel, U. Jacovella, E. Dartois, S. Boyé-Péronne, C. Alcaraz, O. Asvany, S. Brünken, S. Thorwirth, S. Schlemmer, J. R. Goicoechea, G. Rouillé, A. Sidhu, R. Chown, D. Van De Putte, B. Trahin, F. Alarcón, O. Berné, E. Habart, and E. Peeters\\
-**[[https://doi.org/10.1051/0004-6361/202347765|Astronomical CH3+ Rovibrational Assignments &mdash; A Combined Theoretical and Experimental Study Validating Observational Findings in the d203-506 UV-irradiated Protoplanetary Disk]]**\\
+**[[https://doi.org/10.1051/0004-6361/202347765|Astronomical CH3+ Rovibrational Assignments — A Combined Theoretical and Experimental Study Validating Observational Findings in the d203-506 UV-irradiated Protoplanetary Disk]]**\\
 //Astron. Astrophys.// **680**, Art. No. A19 (2023).\\
 Initial spectroscopic parameters were derived from a high-level quantum chemical calculation. The parameters were adjusted through a line-by-line fit of the observational spectrum in spite of the limitations of the latter.\\
 \\
+T. Henning, I. Kamp, M. Samland, A. M. Arabhavi, J. Kanwar, E. F. van Dishoeck, M. Güdel, P.-O. Lagage, C. Waelkens, A. Abergel, O. Absil, D. Barrado, A. Boccaletti, J. Bouwman, A. Caratti o Garatti, V. Geers, A. M. Glauser, F. Lahuis, M. Mueller, C. Nehmé, G. Olofsson, E. Pantin, T. P. Ray, S. Scheithauer, B. Vandenbussche, L. B. F. M. Waters, G. Wright, I. Argyriou, V. Christiaens, R. Franceschi, D. Gasman, S. L. Grant, R. Guadarrama, H. Jang, M. Morales-Calderón, N. Pawellek, G. Perotti, D. Rodgers-Lee, J. Schreiber, K. Schwarz, B. Tabone, M. Temmink, M. Vlasblom, L. Colina, T. R. Greve, and G. Östlin\\
+presented an account on\\
+**[[https://doi.org/10.1088/1538-3873/ad3455|MINDS: The JWST MIRI Mid-INfrared Disk Survey]]**\\
+//Publ. Astron. Soc. Pac.// **136**, Art. No. 054302 (2024).\\
+The methylium cation was detected in the disk of the T Tauri star TW Hya.\\
+\\
+M. Zannese, B. Tabone, E. Habart, E. Dartois, J. R. Goicoechea, L. Coudert, B. Gans, M.-A. Martin-Drumel, U. Jacovella, A. Faure, B. Godard, A. G. G. M. Tielens, R. Le Gal, J. H. Black, S. Vicente, O. Berné, E. Peeters, D. Van De Putte, R. Chown, A. Sidhu, I. Schroetter, A. Canin, and O. Kannavou\\
+found the cation to be more wide-spread in the Orion Bar in their work\\
+**[[https://doi.org/10.1051/0004-6361/202453441|PDRs4All — XI. Detection of infrared CH+ and CH3+ rovibrational emission in the Orion Bar and disk d203-506: Evidence of chemical pumping]]**\\
+//Astron. Astrophys.// **696**, Art. No. A99 (2025).\\
+\\
+C. Bhatt, J. Cami, E. Peeters, N. Clark, P. Moraga Baez, K. Volk, G. C. Sloan, J. H. Kastner, H. L. Dinerstein, M. Matsuura, B. Balick, K. E. Kraemer, K. Justtanont, O. Jones, R. Sahai, I. Aleman, M. J. Barlow, J. Bernard-Salas, J. Blommaert, N. Hirano, P. Kavanagh, F. Kemper, E. Lagadec, J. M. Laming, F. Molster, H. Monteiro, A. M. S. Richards, N. C. Sterling, M. Torki, P. A. M. van Hoof, J. R. Walsh, L. B. F. M. Waters, R. Wesson, F. Wilson, N. J. Wright, and A. A. Zijlstra\\
+reported more recently on\\
+**[[https://doi.org/10.3847/1538-4357/ae1020|Detection of CH3+ in the O-rich Planetary Nebula NGC 6302]]**\\
+//Astrophys. J.// **995**, Art. No. 67 (2025).\\
+\\
 ----