The Binary and the Disk: The Beauty is Found within NGC3132 with JWST by Sahai, Raghvendra, Bujarrabal, Valentin, Quintana-Lacaci, Guillermo, Reindl, Nicole, Van de Steene, Griet, Contreras, Carmen Sánchez, Ressler, Michael E.

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THE ORIGIN OF OB CLUSTERS: FROM 10 pc TO 0.1 pc by HAUYU BAOBAB LIU, QUINTANA-LACACI, Guillermo, KE WANG, HO, Paul T. P, LI, Zhi-Yun, QIZHOU ZHANG, ZHANG, Zhi-Yu

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Atmospheric molecular blobs shape up circumstellar envelopes of AGB stars by Velilla-Prieto, L., Fonfría, J. P., Agúndez, M., Castro-Carrizo, A., Guélin, M., Quintana-Lacaci, G., Cherchneff, I., Joblin, C., McCarthy, M. C., Martín-Gago, J. A., Cernicharo, J.

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Hints of the Existence of C-rich Massive Evolved Stars∗ ∗ Based on observations carried out with the IRAM NOEMA and 30 m. IRAM is supported by INSU/CNRS (France), MPG (Germany) and... by Quintana-Lacaci, Guillermo, Cernicharo, José, Agúndez, Marcelino, Fonfría, José Pablo, Velilla-Prieto, Luis, Contreras, Carmen Sánchez, Bujarrabal, Valentín, Castro-Carrizo, Arancha, Alcolea, Javier

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Hints of the existence of C-rich massive evolved stars by Quintana-Lacaci, Guillermo, Cernicharo, José, Agúndez, Marcelino, Fonfría, José Pablo, Velilla-Prieto, Luis, Contreras, Carmen Sánchez, Bujarrabal, Valentín, Castro-Carrizo, Arancha, Alcolea, Javier

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The binary and the disk: the beauty is found within NGC3132 with JWST by Sahai, Raghvendra, Bujarrabal, Valentin, Quintana-Lacaci, Guillermo, Reindl, Nicole, Griet Van de Steene, Carmen Sánchez Contreras, Ressler, Michael E

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The interplay of dense gas and stars in M33 by Kramer, Carsten, Buchbender, Christof, Quintana-Lacaci, Guillermo, Braine, Jonathan, Gratier, Pierre, Rosolowsky, Erik

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The messy death of a multiple star system and the resulting planetary nebula as observed by JWST by Orsola De Marco, Akashi, Muhammad, Akras, Stavros, Alcolea, Javier, Aleman, Isabel, Amram, Philippe, Balick, Bruce, De Beck, Elvire, Blackman, Eric G, Boffin, Henri M J, Boumis, Panos, Bublitz, Jesse, Bucciarelli, Beatrice, Bujarrabal, Valentin, Cami, Jan, Chornay, Nicholas, You-Hua, Chu, Corradi, Romano L M, Adam, Frank, Garcia-Segura, Guillermo, Garcia-Hernandez, D A, Garcia-Rojas, Jorge, Gomez-Llanos, Veronica, Goncalves, Denise R, Guerrero, Martin A, Jones, David, Karakas, Amanda I, Kastner, Joel H, Sun, Kwok, Lykou, Foteini, Manchado, Arturo, Matsuura, Mikako, McDonald, Iain, Monreal-Ibero, Ana, Monteiro, Hektor, Paula Moraga Baez, Morisset, Christophe, Miszalski, Brent, Mohamed, Shazrene S, Montez, Rodolfo, Nordhaus, Jason, Mendes de Oliveira, Claudia, Osborn, Zara, Otsuka, Masaaki, Parker, Quentin A, Peeters, Els, Quint, Bruno C, Quintana-Lacaci, Guillermo, Redman, Matt, Ruiter, Ashley J, Sabin, Laurence, Carmen Sanchez Contreras, Santander-Garcia, Miguel, Seitenzahl, Ivo, Sahai, Raghvendra, Soker, Noam, Speck, Angela K, Stanghellini, Letizia, Steffen, Wolfgang, Toala, Jesus A, Ueta, Toshiya, Griet Van de Steene, Villaver, Eva, Ventura, Paolo, Vlemmings, Wouter, Walsh, Jeremy R, Wesson, Roger, Hans van Winckel, Zijlstra, Albert A

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The Origin of OB Clusters: From 10 pc to 0.1 pc by Liu, Hauyu Baobab, Quintana-Lacaci, Guillermo, Wang, Ke, Ho, Paul T P, Zhi-Yun, Li, Zhang, Qizhou, Zhang, Zhiyu

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