Page 3: 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.

Two new brown dwarfs discovered with TESS

An international team of astronomers reports the detection of two new brown dwarfs orbiting distant stars using NASA's Transiting Exoplanet Survey Satellite (TESS). The newfound objects are about 30 times more massive than ...

It's twins! Mystery of famed brown dwarf solved

Hundreds of papers have been written about the first known brown dwarf, Gliese 229B, since its discovery by Caltech researchers at the Institute's Palomar Observatory in 1995. But a pressing mystery has persisted about this ...

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