Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

BE Lyncis: A Pulsating Star in the Most Eccentric Binary with a Massive Unseen Companion

  • Authors: Jia-Shu Niu, 家树 牛, Ying Zhang, 颖 张, Hui-Fang Xue, 会芳 薛

Jia-Shu Niu et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 5.

Frequency spectrum of BE Lyn. The main panel (0–100 c day−1) marks the fundamental (f0, red) and first-overtone (f1, green) modes. The inset highlights the low-amplitude, nonradial mode region (∼9–17 c day−1) with a linear y-axis.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse