Objects
Jackson, James M., Whitaker, J. Scott, Rathborne, J. M., Foster, J. B., Contreras, Y., Sanhueza, Patricio, Stephens, Ian W., Longmore, S. N., Allingham, David. Institute of Physics Publishing; 2019. Asymmetric line profiles in dense molecular clumps observed in MALT90: evidence for global collapse.
Whitaker, J. Scott, Jackson, James M., Rathborne, J. M., Foster, J. B., Contreras, Y., Sanhueza, Patricio, Stephens, Ian W., Longmore, S. N.. Institute of Physics Publishing; 2017. MALT90 kinematic distances to dense molecular clumps.
Contreras, Yanett, Sanhueza, Patricio, Sakai, Takeshi, Ohashi, Satoshi, Liu, Tie, Saito, Masao, Gomez, Laura, Rathborne, Jill, Whitaker, Scott, Jackson, James M., Guzmán, Andrés E., Longmore, Steven, Garay, Guido, Zhang, Qizhou, Quang, Nguyễn-Lu'o'ng, Tatematsu, Ken'ichi, Nakamura, Fumitaka. Institute of Physics Publishing (IOP); 2018. Infall signatures in a prestellar core embedded in the high-mass 70 μm Dark IRDC G331.372-00.116.
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.
Sakai, Takeshi, Yanagida, Takahiro, Furuya, Kenji, Aikawa, Yuri, Sanhueza, Patricio, Sakai, Nami, Hirota, Tomoya, Jackson, James M., Yamamoto, Satoshi. Institute of Physics Publishing (IOP); 2018. ALMA observations of the IRDC Clump G34.43+00.24 MM3: complex organic and deuterated molecules.
Jackson, James M., Allingham, David, Killerby-Smith, Nicholas, Whitaker, J. Scott, Smith, Howard A., Contreras, Yanett, Guzman, Andrés E., Hogge, Taylor, Sanhueza, Patricio, Stephens, Ian W.. Institute of Physics (IOP); 2020. Characterizing [C II] line emission in massive star-forming clumps.
Sanhueza, Patricio, Jackson, James M., Zhang, Qizhou, Guzman, Andrés E., Lu, Xing, Stephens, Ian W., Wang, Ke, Tatematsu, Ken'ichi. Institute of Physics Publishing; 2017. A massive prestellar clump hosting no high-mass cores.
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.