📣 Help Shape the Future of UKRI's Gateway to Research (GtR)

We're improving UKRI's Gateway to Research and are seeking your input! Tell us what works, what doesn't, and how we can make GtR more user-friendly, impactful, and effective for the Research and Innovation community. Please send your feedback to gateway@ukri.org by 11 August 2025.

Very regular high-frequency pulsation modes in young intermediate-mass stars (2020)

First Author: Li, Y.

Attributed to: Astronomy Consolidated Grant at UCLAN funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.17615/yxr3-5y93

Publication URI: https://cdr.lib.unc.edu/concern/articles/b8516014x

Type: Other