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The R136 star cluster dissected with Hubble Space Telescope/STIS - II. Physical properties of the most massive stars in R136 (2020)

First Author: Bestenlehner J

Attributed to: Cosmic Impact of Massive Stars: Mass Loss and Mixing funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staa2801

Publication URI: http://dx.doi.org/10.1093/mnras/staa2801

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 2