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arXiv · 2309.01084

Rotational Variability and Detection of Superflares in a Young Brown Dwarf by TESS

Rajib Kumbhakar·Soumen Mondal·Samrat Ghosh·Diya Ram·Sudip Pramanik
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Abstract

We present a comprehensive analysis of a Transiting Exoplanet Survey Satellite (TESS) high-quality light curve for a young brown dwarf, MHO~4 having spectral type M7.0, in the Taurus star-forming region. We investigate the rotation periods and characterize the BD's dynamic atmosphere and surface features. We present light curve analysis of MHO~4, and estimate the rotation period to be around 2.224~d. Remarkably, MHO~4 exhibits two significant flaring events. Furthermore, we also estimated bolometric flare energies to be within the energy range of $10^{34}$ to $10^{35}$ erg, which sits in the superflare category.

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Rajib Kumbhakar, Soumen Mondal, Samrat Ghosh, Diya Ram, Sudip Pramanik. 2023-09-03. Rotational Variability and Detection of Superflares in a Young Brown Dwarf by TESS. https://arxiv.org/abs/2309.01084

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