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The orbit of HD 142527 B is too compact to explain many of the disc features (2024)

First Author: Nowak M

Attributed to: Astrophysics Research at the University of Leicester funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2402.03595

Publication URI: https://arxiv.org/abs/2402.03595

Type: Preprint