Figure 4 from Runaway Stars as Possible Sources of the Elliptical Ring Structures in NGC 7538

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Runaway Stars as Possible Sources of the Elliptical Ring Structures in NGC 7538

Authors: Josephine Fenske, Jason Arakawa, Cassandra Fallscheer, and James Di Francesco

2021 The Astronomical Journal 161 156.

Provider: AAS Journals

Caption: Figure 4.

Candidate star BD +61 2408's motion shown from a face-on perspective to show that the star was likely, at some point in the past, coincident with the northern ring’s center. All other aspects of this figure are identical to Figure 3.

Other Images in This Article

Copyright and Terms & Conditions