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Dense Molecular Clumps with Large Blue Asymmetries: Evidence for Collapse

  • Authors: James M. Jackson, J. Scott Whitaker, Edward Chambers, Robert Simon, Cristian Guevara, David Allingham, Philippa Patterson, Nicholas Killerby-Smith, Jacob Askew, Patricio Sanhueza, Ian W. Stephens, Anika Schmiedeke, Robert Loughnane

James M. Jackson et al 2026 The Astrophysical Journal 998 .

  • Provider: AAS Journals

Caption: Figure 25.

Simulated line profiles of HCO+ (1–0) in a simple two-cloud model. The blue vertical lines represent the velocity of the warm background cloud and the red vertical lines the velocity of the cold foreground cloud. The profiles show a grid of various foreground cloud optical depths and velocity offsets, with foreground cloud optical depth ranging from 1 to 16, varying by factors of 2 (y-direction) and offset velocities V2 − V1 ranging from −2 to 12 km s−1, in steps of 2 km s−1 (x-direction). Parameters for this particular model are shown in the title. The line profiles show skewed, blue asymmetries for large foreground optical depths and velocity offsets of ∼2–8 km s−1, shown in the lower-middle panels in the plot.

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