Image Details

Choose export citation format:

SPYGLASS. V. Spatially and Temporally Structured Star-forming Environments in the Cepheus-Hercules Complex

  • Authors: Ronan Kerr, Adam L. Kraus, Daniel Krolikowski, Luke G. Bouma, Juan P. Farias

Ronan Kerr et al 2024 The Astrophysical Journal 975 .

  • Provider: AAS Journals

Caption: Figure 3.

Results of RV selection across a cross section of space and velocity axes in Cep-Her Main (top) and Cep-Her North (bottom). Dark blue diamonds are accepted as kinematic members, and light blue dots are not. For the plots of velocity against galactic l coordinates, we use a red curve to show the median values of U, V, and W as a function of l, which were used to define the velocity loci for the two subtly discontiguous subcomponents of Cep-Her. The shaded red region encloses the maximum and minimum velocities, which may be identified as members in that axis, as defined by the velocity axis, plus or minus the maximum velocity dispersion.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse