Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

Proper Motion of Dense Circumstellar Knots in the Supernova Remnant Cassiopeia A

  • Authors: Bon-Chul Koo, Sang Bum Ko, Christopher F. McKee, Carl Heiles, Robert A. Fesen, Ji Yeon Seok, Hyun-Jeong Kim, Sung-Chul Yoon

Bon-Chul Koo et al 2025 The Astrophysical Journal Supplement Series 280 .

  • Provider: AAS Journals

Caption: Figure 5.

(a) R.A. component of the proper motion of QSFs vs. their projected distance from the expansion center along R.A. The solid line represents the least-squares fit. (b) Same as (a), but for the decl. component of the proper motion. Blue symbols indicate Group 1 QSFs, while magenta symbols represent Group 2 QSFs.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse