Dwarf carbon stars are likely metal-poor binaries and unlikely hosts to carbon planets (2018)

First Author: Whitehouse L

Attributed to: UCL Astrophysics Consolidated Grant 2018-2021 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/sty1622

Publication URI: http://dx.doi.org/10.1093/mnras/sty1622

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 3