Research Topic

The Future of Asteroseismology

About this Research Topic

Asteroseismology offers the exciting prospect of being able to see inside stellar interiors by observing global oscillation modes. The field of asteroseismology has experienced a prolific two decades resulting from the influx of data from ground-based networks such as WET, OGLE, ASAS, DSN, and space missions ...

Asteroseismology offers the exciting prospect of being able to see inside stellar interiors by observing global oscillation modes. The field of asteroseismology has experienced a prolific two decades resulting from the influx of data from ground-based networks such as WET, OGLE, ASAS, DSN, and space missions such as MOST, BRITE, CoRoT, Kepler, K2, soon to be followed by TESS and PLATO.

The purpose of this volume is not only to take stock of accomplishments and barriers to further progress, and but also to assess prospects for future breakthroughs in asteroseismology, even as the methods of doing science are being challenged and transformed by changes in communications and collaboration, massively parallel computing, automated data processing, machine learning, and evolving priorities among various fields of research.

The aim of this Research Topic is to be speculative and even controversial, and to provoke brainstorming and creativity in this field. We intend this volume to be a resource for research advisors and students to inspire new projects and directions. Authors are encouraged to address key questions, challenges, and barriers to progress in each area, and to outline ideas for new data, advances in physics models or computational simulations to address them.

A list of possible, not exhaustive, topical areas follows:

1) Theory and simulation; stellar evolution and pulsation modeling
2) Model atmospheres
3) Stellar abundances
4) What is your ‘wish list’ for asteroseismic data?
5) Dealing with large datasets
6) Binary, disk, and multiple star effects
7) Mode amplitude and selection
8) New pulsation driving mechanisms; undiscovered/unverified variable star types
9) Seismology of astrophysical objects (e.g. stellar disks, giant planets)
10) Constraints on supernova progenitors (e.g. LBVs, RSGs, Be stars)
11) How can asteroseismology inform helioseismology (and vice versa)?
12) How could asteroseismology benefit from an interdisciplinary or multidisciplinary approach? Why is this field important? What is its ambition? What is the impact and relative importance of this field compared to other sub-disciplines of astrophysics?


Keywords: Stellar pulsation, Stellar evolution, Asteroseismology, Stellar interior, Stellar structure


Important Note: All contributions to this Research Topic must be within the scope of the section and journal to which they are submitted, as defined in their mission statements. Frontiers reserves the right to guide an out-of-scope manuscript to a more suitable section or journal at any stage of peer review.

Recent Articles

Loading..

About Frontiers Research Topics

With their unique mixes of varied contributions from Original Research to Review Articles, Research Topics unify the most influential researchers, the latest key findings and historical advances in a hot research area! Find out more on how to host your own Frontiers Research Topic or contribute to one as an author.

Topic Editors

Loading..

Submission Deadlines

18 January 2019 Manuscript

Participating Journals

Manuscripts can be submitted to this Research Topic via the following journals:

Loading..

Topic Editors

Loading..

Submission Deadlines

18 January 2019 Manuscript

Participating Journals

Manuscripts can be submitted to this Research Topic via the following journals:

Loading..
Loading..

total views article views article downloads topic views

}
 
Top countries
Top referring sites
Loading..

Comments

Loading..

Add a comment

Add comment
Back to top
);