Objects
Hogge, Taylor G., Jackson, James M., Allingham, David, Guzman, Andres E., Killerby-Smith, Nicholas, Kraemer, Kathleen E., Sanhueza, Patricio, Stephens, Ian W., Whitaker, J. Scott. Institute of Physics; 2019. The interaction between the supernova remnant W41 and the filamentary infrared dark cloud G23.33-0.30.
Jackson, James M., Contreras, Yanett, Rathborne, Jill M., Whitaker, J. Scott, Guzman, Andrés, Stephens, Ian W., Sanhueza, Patricio, Longmore, Steven, Zhang, Qizhou, Allingham, David. Institute of Physics Publishing (IOP); 2018. G337.342-0.119 (The "Pebble"): A cold, dense, high-mass molecular cloud with unusually large line widths and a candidate high-mass star cluster progenitor.
Sabatini, Giovanni, Bovino, Stefano, Izumi, Natsuko, Sakai, Takeshi, Tatematsu, Ken'ichi, Allingham, David, Sanhueza, Patricio, Morii, Kaho, Li, Shanghuo, Redaelli, Elena, Zhang, Qizhou, Lu, Xing, Feng, Siyi, Tafoya, Daniel. Institute of Physics Publishing inc.; 2022. The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). VI. The Core-scale CO Depletion.
Li, Shanghuo, Sanhueza, Patricio, Tafoya, Daniel, Tatematsu, Ken'ichi, Sakai, Takeshi, Wang, Junzhi, Li, Fei, Silva, Andrea, Izumi, Natsuko, Allingham, David, Lu, Xing, Lee, Chang Won, Zhang, Qizhou, Bovino, Stefano, Sabatini, Giovanni, Liu, Tie, Kim, Kee-Tae, Morii, Kaho. Institue of Physics (IOP); 2022. The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). VII. Chemistry of Embedded Dense Cores.