Independent Study and Spectral Classification of a Sample of Poorly Studied High Proper Motion M-dwarf Candidate Stars

TL;DR

This study independently classifies poorly studied high proper motion M-dwarf stars using spectral data, aiding exoplanet research and stellar population models by providing crucial stellar properties.

Contribution

It offers new spectral classifications for a sample of M-dwarfs, serving as an independent validation and contributing to stellar and exoplanetary studies.

Findings

33% of stars show Halpha emission

Evidence of Halpha variability in one star

Spectral classification aids in exoplanet and stellar population studies

Abstract

We report an independent spectral classification of a sample of poorly studied M-dwarf candidate stars observed with the OSIRIS instrument at GTC. Our project was carried out as an independent test of the spectral classification. It is crucial for the studies of extrasolar planets orbiting M-dwarfs, since properties of the host star are directly related to understanding the planet properties and possible habitability. Understanding of the statistical properties of the dwarf stars is also crucial for the Simple Stellar Population models that play a major role in the modern astrophysics. Halpha emission was detected in 33% of the sample with evidence of Halpha variability in one object.