The Lifecycle of Massive Stars

A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Solar and Stellar Physics".

Deadline for manuscript submissions: closed (1 August 2026) | Viewed by 1085

Editor


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Guest Editor
Lennard-Jones Laboratories, Keele University, Keele, Newcastle ST5 5BG, UK
Interests: evolved stars; stellar mass loss; supernova remnants; masers; dust; interstellar medium; galaxy evolution; active galactic nuclei
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Special Issue Information

Dear Colleagues,

We invite you to submit focused reviews, original analyses or novel ideas pertaining to the formation, evolution and death of massive stars. By publishing in this Special Issue of Universe, your work will receive more visibility. As Guest Editor, I am committed to providing guidance and support to anyone who would appreciate it, as well as to helping scientists from under-represented or underserved communities join an inclusive massive star community.

We welcome the speculative interrogation of open problems and proposals for new research avenues, as well as cross-disciplinary discussions of available evidence and current thinking regarding the fundamental structure, dynamics and environmental interaction of massive stars and their role in the evolution of the baryonic universe. If you are unsure whether your proposed paper would fit the scope of this Special Issue, titled “The Lifecycle of Massive Stars”, please do not hesitate to contact us.

Best wishes,

Dr. Jacco Th. van Loon
Guest Editor

Manuscript Submission Information

Manuscripts should be submitted online at www.mdpi.com by registering and logging in to this website. Once you are registered, click here to go to the submission form. Manuscripts can be submitted until the deadline. All submissions that pass pre-check are peer-reviewed. Accepted papers will be published continuously in the journal (as soon as accepted) and will be listed together on the special issue website. Research articles, review articles as well as short communications are invited. For planned papers, a title and short abstract (about 250 words) can be sent to the Editorial Office for assessment.

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Keywords

  • massive stars
  • star formation
  • stellar evolution
  • stellar mass loss
  • stellar winds
  • supernova progenitors
  • binary stars
  • stellar magnetism
  • stellar rotation
  • population III

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Published Papers (1 paper)

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Review

16 pages, 1435 KB  
Review
The Complex Upper HR Diagram—Redux: The Low-Metallicity Galaxies
by Roberta M. Humphreys
Universe 2026, 12(8), 229; https://doi.org/10.3390/universe12080229 - 31 Jul 2026
Viewed by 255
Abstract
The properties of luminous evolved stars in nearby resolved galaxies are briefly reviewed with emphasis on recent results for the low-metallicity dwarf irregulars. Highlights and recent discoveries of some of the more extreme examples with high rates of mass loss such as the [...] Read more.
The properties of luminous evolved stars in nearby resolved galaxies are briefly reviewed with emphasis on recent results for the low-metallicity dwarf irregulars. Highlights and recent discoveries of some of the more extreme examples with high rates of mass loss such as the yellow and red hypergiants, LBVs, and giant eruptions are summarized. Some of the most interesting new results are the evidence for high-luminosity stars at high redshift and at very low metallicities with mass loss. The presence of an empirical upper luminosity limit at very low metallicities similar to what we observe in the Milky Way and Local Group galaxies is presented. Its implications for the first stars in the early Universe and mass loss mechanisms at very low metallicity are discussed. Full article
(This article belongs to the Special Issue The Lifecycle of Massive Stars)
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