Special Issue "Luminous Stars in Nearby Galaxies"
A special issue of Galaxies (ISSN 2075-4434).
Deadline for manuscript submissions: 30 June 2019
Prof. Roberta M. Humphreys
School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455, USA
Interests: massive stars, giant eruptions, supernova impostors, stellar populations
Perhaps the greatest uncertainty in all of astrophysics and especially in stellar structure and evolution, is distance. This is especially true for the most massive, most luminous stars that may be at very large distances in our own galaxy. Studies of stellar populations in nearby galaxies thus have the advantage that all the stars are at the approximately the same distance, a distance that is relatively well known, especially in comparison with the uncertain distances of individual stars in our own galaxy. Surveys and the subsequent spectroscopy of massive stars in different stages of stellar evolution in the relatively nearby resolved galaxies have revealed a complex distribution in the luminosity–temperature plane, the HR Diagram. The fundamentals of massive star evolution are basically understood, but the roles of mass loss, episodic mass loss, rotation, and binarity are still in question. The final stages of these stars of different masses and their possible relation to each other are not understood. The purpose of this volume is a current review of the different populations of evolved massive stars. The emphasis is on massive stars in the Local Group; the Magellanic Clouds and the nearby spirals M31 and M33.
Prof. Roberta M. Humphreys
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 papers will be 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 100 words) can be sent to the Editorial Office for announcement on this website.
Submitted manuscripts should not have been published previously, nor be under consideration for publication elsewhere (except conference proceedings papers). All manuscripts are thoroughly refereed through a single-blind peer-review process. A guide for authors and other relevant information for submission of manuscripts is available on the Instructions for Authors page. Galaxies is an international peer-reviewed open access quarterly journal published by MDPI.
Please visit the Instructions for Authors page before submitting a manuscript. The Article Processing Charge (APC) for publication in this open access journal is 350 CHF (Swiss Francs). Submitted papers should be well formatted and use good English. Authors may use MDPI's English editing service prior to publication or during author revisions.
- massive stars
- stellar evolution
- mass loss
- Magellanic Clouds
The below list represents only planned manuscripts. Some of these manuscripts have not been received by the Editorial Office yet. Papers submitted to MDPI journals are subject to peer-review.
Luminous Blue Variables -- Kerstin Weis and Domink Bomans, Bochum University, Germany
B[e] Supergiants -- Michaela Kraus, Astronomical Institut, Czech Republic
Wolf-Rayet Stars -- Phil Massey and Kathryn Neugent , Lowell Obs., Arizona
Luminous Hot Stars, Large Magellanic Cloud – Paul Crowther, Sheffield University, UK
Hypergiants and Post Red Supergiant Evolution – Michael Gordon and R. Humphrey