Image Details

Choose export citation format:

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 22.

Top left: the asymmetry parameter A for HCN (1–0) versus the asymmetry parameter A for HCO+ (1–0), using N2H+ (1–0) as the reference line. Top right: the asymmetry parameter A for HNC (1–0) versus the asymmetry parameter A for HCO+ (1–0), using N2H+ (1–0) as the reference line. Bottom left: the asymmetry parameter A for C2H (N = 1–0; J = 3/2–1/2; F = 2–1), versus the asymmetry parameter A for HCO+ (1–0), using N2H+ (1–0) as the reference line. Bottom right: the asymmetry parameter A for H13CO+ (1–0) versus the asymmetry parameter A for HCO+ (1–0), using N2H+ (1–0) as the reference line. For all plots, the orange diagonal line represents equal values of A for both lines. The dotted gray lines indicate values of A = 0 for both lines. The plotted uncertainties are σtot, as described in the text. All of these lines typically have positive values for A. The largest values of A occur for HCO+. As the optical depth decreases, the values of A also decrease.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse