Image Details

Choose export citation format:

Three‐dimensional Structure of the Milky Way Disk: The Distribution of Stars and Dust beyond 0.35 R

  • Authors: Ronald Drimmel and David N. Spergel

Drimmel & Spergel 2001 The Astrophysical Journal 556 181.

  • Provider: AAS Journals

Caption: Fig. 19.

Schematic of the Galaxy showing the four spiral arms as mapped by H II regions and the dust (bold lines), the sheared arms in the K band (stars), and the arms in the two‐arm logarithmic model for J‐ and K‐band fit (dashed) and the K‐band fit alone (solid) (Drimmel, & Spergel 2001). The H II spirals are incomplete on the opposite side of the Galaxy owing to lack of data.

Other Images in This Article

Show More

Copyright and Terms & Conditions