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Open Astronomy

formerly Baltic Astronomy

Editor-in-Chief: Barbuy, Beatriz


IMPACT FACTOR 2018: 0.350

CiteScore 2018: 0.24

SCImago Journal Rank (SJR) 2018: 0.202
Source Normalized Impact per Paper (SNIP) 2018: 0.144

ICV 2018: 120.66

Open Access
Online
ISSN
2543-6376
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Volume 21, Issue 1-2

Issues

Multiwavelength SED as a Tool in Understanding Outbursts of Symbiotic Binaries

A. Skopal
Published Online: 2017-03-23 | DOI: https://doi.org/10.1515/astro-2017-0363

Abstract

Symbiotic binaries consist of a few sources of radiation contributing to spectral energy distribution (SED) from hard X-rays to radio wavelengths. To identify the basic physical processes forming the observed spectrum, we have to disentangle the composite SED into its individual components of radiation, i.e., to determine their physical parameters. Spectral disentangling of different objects at different stages of activity allows us to understand the mechanism of their outbursts. In this contribution I demonstrate the method of multiwave-length modeling SEDs on the example of two classical symbiotic stars, AG Dra and Z And.

Keywords: stars; binaries; symbiotic; X-rays; binaries; stars; fundamental parameters

References

About the article

Received: 2011-09-01

Accepted: 2011-09-15

Published Online: 2017-03-23

Published in Print: 2012-06-01


Citation Information: Open Astronomy, Volume 21, Issue 1-2, Pages 97–104, ISSN (Online) 2543-6376, DOI: https://doi.org/10.1515/astro-2017-0363.

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© 2017. This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 License. BY-NC-ND 4.0

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