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Simulations of stellar winds from X-ray bursts: Characterization of solutions and observable variables.

Author
Herrera, Y.; Sala, G.; Jose, J.
Type of activity
Journal article
Journal
Astronomy and astrophysics
Date of publication
2020-06-19
Volume
638
First page
1
Last page
10
DOI
10.1051/0004-6361/201936895
Repository
http://hdl.handle.net/2117/338375 Open in new window
URL
https://www.aanda.org/articles/aa/abs/2020/06/aa36895-19/aa36895-19.html Open in new window
Abstract
Context. Photospheric radius expansion during X-ray bursts can be used to measure neutron star radii and help constrain the equation of state of neutron star matter. Understanding the stellar wind dynamics is important for interpreting observations, and therefore stellar wind models, though studied in past decades, have regained interest and need to be revisited with updated data and methods. Aims. Here, we study the radiative wind model in the context of X-ray bursts with modern techniques and ...
Citation
Herrera, Y.; Sala, G.; Jose, J. Simulations of stellar winds from X-ray bursts: Characterization of solutions and observable variables. "Astronomy and astrophysics", 19 Juny 2020, vol. 638, p. 1-10.
Keywords
Methods: numerical, Stars: neutron, Stars: winds, outflows, X-rays: bursts
Group of research
GAA - Astronomy and Astrophysics Group

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