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Optical morphology of the ejected Shell of V339 Del using SHAPE
Author(s) -
S. Sutham,
J. Sobbong,
F. Surina,
S. Awipan
Publication year - 2019
Publication title -
journal of physics. conference series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.21
H-Index - 85
eISSN - 1742-6596
pISSN - 1742-6588
DOI - 10.1088/1742-6596/1380/1/012029
Subject(s) - morphology (biology) , shell (structure) , astrophysics , line (geometry) , spectral line , physics , torus , telescope , emission spectrum , optics , materials science , astronomy , geometry , geology , mathematics , composite material , paleontology
The morphology of the ejected shell of V339 Del (Nova Del 2013) outburst was preliminary studied. The optical spectra from the Liverpool telescope around 80 days after discovery were examined. Synthetic line profile spectra were compared to emission lines of H β in order to find the best-fit morphology of the ejected shell using the programme SHAPE. When adopted an inclination i = 65° and suggested shape of the shell from literature, a simplest preliminary morphology was found to be a bipolar at squeeze parameter around 0.8 - 1 with a torus.

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