Special Issue "Astrophysics of Eclipsing Binaries in the Era of Space-Borne Telescopes"
A special issue of Galaxies (ISSN 2075-4434).
Deadline for manuscript submissions: closed (1 July 2022) | Viewed by 10110
Interests: eclipsing binary evolution models; optical instrumentation and space optics; stellar occultations by asteroids TNO and KPO objects; exoplanets; long-term monitoring of blazars
Eclipsing binaries are one of the most efficient tools in stellar astrophysics and they play an important role in the investigation of certain evolution channels. In parallel, space-borne telescopes offer a wealth of information on stellar astrophysics, exoplanets, and multiple system dynamics. Today, high-accuracy astrometric and photometric data are available, while the space era opens a new window in the science of eclipsing binaries. The impact of large photometric surveys and big data statistics in stellar evolution is huge, and specially designed tools for analyzing the vast number of discovered systems are being developed and lead towards a new way of stellar modeling. The formation and evolution of massive binaries, low-temperature contact binaries, and stellar merger candidates are some of the unresolved issues in modern stellar evolution. In addition, the discovery of circumbinary planets shed light on the planetary formation environment and properties. On the other hand, asteroseismology and stellar pulsations triggered in binary and multiple systems offer a unique opportunity to study stellar interior and investigate the invisible stellar structure.
The aim of this Special Issue is to review and present the most modern knowledge on eclipsing binary studies in the era of space-borne telescopes, robotic sky surveys, and artificial intelligence pipelines and data reduction processes. Special emphasis is given to understanding the physical properties, structure, and evolution of stars within stellar systems, which, in turn, will lead to knowledge of the origin of eclipsing binaries through their stellar progenitors. Some of the key topics to be covered are outlined in the following list:
- Eclipsing binaries in the GAIA era
- Large photometric surveys on eclipsing binaries
- Formation and evolution of binary systems – stellar mergers
- Circumbinary planets
- Magnetically active binaries
- Pulsation in binaries
- New approaches to physical modeling of binary stars
Submission of reviews, as well as focused research articles, are welcome!
Prof. Kosmas Gazeas
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. Galaxiesis an international peer-reviewed open access quarterly journal published by MDPI.
Please visit the Instructions for Authors page before submitting a manuscript. 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.
- eclipsing binaries
- stellar evolution
- space-borne data
- photometric surveys
- planetary systems in binary stars
- artificial intelligence and automatic pipelines for eclipsing binary processing