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 2.

Hertzsprung–Russell diagram showing evolutionary tracks (colored solid lines from the zero-age main sequence, ZAMS, to post-MS) and the best-fit seismic model for BE Lyn’s primary (red star). Black rectangles highlight zoomed-in views around the best-fit solutions. Colored dashed lines indicate tracks with a 0.01M⊙ mass step.

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