Abstract

We report on the results of our low resolution spectroscopic observations during the 2011 outburst of the recurrent nova T Pyx. Our observations were performed from 0.19 days to 34 days after the eruption discovered by M. Linnolt. We found Wolf-Rayet like features in our spectrum during the initial rising phase on <em>t</em> = 0.19 d. Following spectral developments are consistent with previous works. We discuss that the early phase of T Pyx is divided into three stages, a short lived WR-like stage, He/N stage and Fe II stage.

Highlights

  • The initial rising phase of novae is a very intriguing phase in the point of view of thermonuclear runaway and development of spectral features

  • Low resolution spectroscopic observations in past outbursts were performed around their visual maximum (e.g., Adams and Joy 1920, Joy 1945, and Catchpole et al 1969)

  • Recurrent novae are classified into three types, the U Sco, the RS Oph- and the T Pyx-types, based on the light curves and spectroscopic features (Anupama et al 2008)

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Summary

Introduction

The initial rising phase of novae is a very intriguing phase in the point of view of thermonuclear runaway and development of spectral features. The study in the early spectroscopic observations and photometry revealed that T Pyx showed rare hybrid spectral classification types (Williams 1992), He/N - Fe II - He/N transition (e.g. Izzo et al 2012, Imamura and Tanabe 2012, Surina et al 2014). We focused on the Wolf-Rayet feature in the initial rising phase on t = 0.19 d (2011 April 14.48) and following developments of spectral features from t = 2 d to t = 34 d.

Results
Conclusion
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