English

(Sub-)stellar variability: from 20 M$_{\odot}$ to 13 M$_{\rm Jup}$

Solar and Stellar Astrophysics 2016-04-22 v1

Abstract

Massive early-type stars vary; low-mass late-type brown dwarfs vary, too. I will make a short, but illustrative, summary of my previous studies on stellar and sub-stellar photometric variability (including the discovery of the most variable brown dwarf in the whole sky), and explain how amateurs can help professional astronomers with our investigations.

Keywords

Cite

@article{arxiv.1604.06128,
  title  = {(Sub-)stellar variability: from 20 M$_{\odot}$ to 13 M$_{\rm Jup}$},
  author = {J. A. Caballero},
  journal= {arXiv preprint arXiv:1604.06128},
  year   = {2016}
}

Comments

Published in "Proceedings of the 47th Conference on Variable Stars Research", Variable Star and Exoplanet Section of Czech Astronomical Society, 27-29 Nov 2015, Ostrava Planetarium, Ostrava, Czech Republic

R2 v1 2026-06-22T13:37:20.749Z