Characterizing [C II] line emission in massive star-forming clumps

- 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.

Asymmetric line profiles in dense molecular clumps observed in MALT90: evidence for global collapse

- Jackson, James M., Whitaker, J. Scott, Rathborne, J. M., Foster, J. B., Contreras, Y., Sanhueza, Patricio, Stephens, Ian W., Longmore, S. N., Allingham, David

The interaction between the supernova remnant W41 and the filamentary infrared dark cloud G23.33-0.30

- 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

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

- Jackson, James M., Contreras, Yanett, Rathborne, Jill M., Whitaker, J. Scott, Guzman, Andrés, Stephens, Ian W., Sanhueza, Patricio, Longmore, Steven, Zhang, Qizhou, Allingham, David

MALT90 kinematic distances to dense molecular clumps

- Whitaker, J. Scott, Jackson, James M., Rathborne, J. M., Foster, J. B., Contreras, Y., Sanhueza, Patricio, Stephens, Ian W., Longmore, S. N.