Search

Image Details

View Article Bookmark & Share

Choose export citation format:

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

Discovery and Timing of Pulsars in the Globular Cluster M13 with FAST

  • Authors: Lin Wang, Bo Peng, B. W. Stappers, Kuo Liu, M. J. Keith, A. G. Lyne, Jiguang Lu, Ye-Zhao Yu, Feifei Kou, Jun Yan, Peng Jiang, Chengjin Jin, Di Li, Qi Li, Lei Qian, Qiming Wang, Youling Yue, Haiyan Zhang, Shuxin Zhang, and Yan Zhu

2020 The Astrophysical Journal 892 43.

  • Provider: AAS Journals

Caption: Figure 8.

Eccentricity vs. orbital period of all binary pulsars. Black crosses are pulsars in the Galactic plane, green triangles are pulsars in GCs (except M13), and red squares are binary pulsars in M13. The data used in this figure are from the ATNF Pulsar Catalog (https://www.atnf.csiro.au/research/pulsar/psrcat/)(Manchester et al. 2005).

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
Copyright and Terms & Conditions

Additional terms of reuse