properties of recurrent nova t pyxidis based on 2011 outburst

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ID: 252439
2015
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Abstract
We reexamine the properties of the recurrent nova T Pyxidis based on our own spectroscopic data accompanying with the photometric ones by VSOLJ (Variable Star Observers League in Japan) during 2011 outburst. One of the purpose of this paper is whether a missing outburst could be happen around 1988-1989. Comparing the 2011 outburst data with previous ones, we may conclude that any essential difference can not be found. Accordingly it is difficult to deny a small possibility of a ”missing” outburst from 1988 to 1989, taking into account the seasonal gap in its observation for northern hemisphere observers . The problem whether IM Normae belongs to be a member of T Pyx subclass or not is to be postponed by its next outburst taking into account of T Pyx’s peculiar spectral behavior.
Reference Key
tanabe2015actaproperties Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors ;K. Tanabe
Journal BMC Bioinformatics
Year 2015
DOI
10.14311/APP.2015.02.0261
URL
https://ojs.cvut.cz/ojs/index.php/APP/article/view/2917
Keywords
engineering (general) civil engineering (general)

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