Temperatture esttiimattiion off EXDRA and SSUMI dwarff Nova systtems from spectroscopic data

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Temperatture esttiimattiion off EXDRA and SSUMI dwarff Nova systtems from spectroscopic data
Published: Feb 4, 2019
DOI: https://doi.org/10.30723/ijp.v13i27.261
Keywords:
Dwarf Nova, Fourier Model, transform and mathematical modeling.

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Arshed Ali Kadhem

Abstract

The seasonal behavior of the light curve for selected star SS UMI and EXDRA during outburst cycle is studied. This behavior describes maximum temperature of outburst in dwarf nova. The raw data has been mathematically modeled by fitting Gaussian function based on the full width of the half maximum and the maximum value of the Gaussian. The results of this modeling describe the value of temperature of the dwarf novae star system leading to identify the type of elements that each dwarf nova consisted of.

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How to Cite
1.
Kadhem AA. Temperatture esttiimattiion off EXDRA and SSUMI dwarff Nova systtems from spectroscopic data. IJP [Internet]. 2019 Feb. 4 [cited 2024 Dec. 19];13(27):31-5. Available from: https://ijp.uobaghdad.edu.iq/index.php/physics/article/view/261
Issue
Vol. 13 No. 27 (2015)
Section
Articles
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This work is licensed under a Creative Commons Attribution 4.0 International License.

© 2023 The Author(s). Published by College of Science, University of Baghdad. This is an open-access article distributed under the terms of the Creative Commons Attribution 4.0 International License. 

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