Research news on Brown dwarfs

Brown dwarf research is a subfield of astrophysics focused on objects with masses between the heaviest gas giant planets and the lightest stars, insufficient to sustain stable hydrogen fusion. This research area investigates their formation pathways, atmospheric chemistry and dynamics, internal structure, cooling and evolutionary tracks, and spectral classification (e.g., L, T, and Y types). It leverages multiwavelength observations, high-resolution spectroscopy, and theoretical modeling to constrain substellar mass functions, metallicities, cloud physics, and magnetic activity, and to calibrate brown dwarfs as analogs for exoplanet atmospheres and as benchmarks for testing low-temperature equation-of-state and radiative-transfer models.

How two dim stars came together to shine brightly

Brown dwarfs get a bad rap in the stellar world, often labeled as "failed stars" for their inability to sustain nuclear fusion at their cores. The mass of these objects falls between planets and stars, ranging from 13 to ...

Rare brown dwarf discovered orbiting ancient star

Astronomers from the Harvard-Smithsonian Center for Astrophysics (CfA) and elsewhere report the discovery of a new brown dwarf about 60 times more massive than Jupiter. The newfound substellar object, designated TOI-7019 ...

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