A light curve model for the Nova V5116-Sgr

A light curve model for the Nova V5116-Sgr

To access the full text documents, please follow this link:: http://hdl.handle.net/2117/191099
Other authors: Sala Cladellas, Glòria
Date: 2021-03-25
Document type: Coursework
Published by: Universitat Politècnica de Catalunya

Note:

 
We develop a light curve model of the emission of both optical and X-ray light of a binary system with a white dwarf, a secondary main-sequence star and an accretion disk. We fit our model to the observational X-ray and optical data of V5116-Sgr.
 
2014/2015
 
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