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{{Short description|Brown dwarf in the constellation Chamaleon}} ...3=Bromm|first3=Volker|date=May 2002|title=The formation mechanism of brown dwarfs|journal=MNRAS|language=en|volume=332|issue=3|pages=L65–L68|doi=10.1046/j.13 ...

{{Short description|Brown dwarf in the constellation Taurus}} ...its [[magnetic field]], as observed in other known rapidly-rotating brown dwarfs.<ref name="Tannock2021"/> ...

{{Short description|Brown dwarf in the constellation Coma Berenices}} ...its [[magnetic field]], as observed in other known rapidly-rotating brown dwarfs.<ref name="Tannock2021"/> ...

{{Short description|Brown dwarf in the constellation Libra}} |caption= "The Accident" brown dwarf in motion ([[Wide-field Infrared Survey Explorer|WISE]] ...

|type=[[brown dwarf]] ...ss|M_J]]}}, which makes this object a [[brown dwarf]] or a [[sub-brown dwarf]], with a temperature of 700 to 900 K.<ref name="Lodieu et al" /> A s ...

{{short description|Brown dwarf}} ...rcumstellar disc]]{{mdash}}as of April 2023, it is one of only two known [[brown dwarf]]s to do so.<ref name="Zhang2023"/> Separated by roughly {{convert|20 ...

| class = G1V<ref name="MKclass"/> / G3V<ref name="MKclass"/> / L8 <ref name="brown"/> ...[[light-year]]s away. The primary component is a mid-wide binary, while a brown dwarf component is located at a wide separation. ...

[[File:2022 229 Display.jpg|thumb|Exoplanet and Brown Dwarf Models displayed at Clifton Park Museum.]] ...projects as an independent scholar, including work with exoplanets, brown dwarfs, comets and Mars. He was a member of South Yorkshire's [[Mexborough and Swi ...

| color = Black, reddish brown, pale yellow, yellowish orange === In stars and brown dwarfs === ...

{{Short description|Sub-brown dwarf in the constellation Hydra}} | type = [[Sub-brown dwarf]] ...

...tance and period of one of its [[natural satellite|satellites]],<ref name="Brown Schaller 2007" /> advanced [[astrometry]] techniques that use the motions o ....<ref name="minimum" /><ref name=bbc20060818/> Smaller bodies are called [[brown dwarf]]s, which occupy a poorly defined grey area between stars and [[gas g ...

...lest exoplanet to be directly imaged, and cooler than all but one imaged [[brown dwarf]] (the exception being the planetary-mass [[WISE 0855−0714]]).<ref na ...es a benchmark case for the study of the formation of gas giants and brown dwarfs.<ref name="Feng2018"/> ...

| type2 = [[Brown dwarf]]<ref name=Meshkat2015/><ref name=Franson2022/> ...a young star, estimated 30 to 200 million years old, and is orbited by a [[brown dwarf]] companion. [[Parallax]] measurements by the [[Gaia (spacecraft)|Gai ...

...ith the [[Y dwarf|spectral type Y]]. They are a mix of [[Brown dwarf|brown dwarfs]] and [[Rogue planet|planetary-mass objects]]. They are the coldest such ob |+List of Y-dwarfs ...

=== Black dwarfs === === White dwarfs === ...

...a spectrum similar to early [[L dwarf|L-dwarfs]], but redder than field L-dwarfs.<ref name="Delorme2013"/> In 2020 Eriksson et al. discovered Hydrogen-alpha ...a [[circumstellar disk]].<ref name="Betti2022"/> Giant planets and [[brown dwarfs]] are thought to form via disk fragmentation in rare cases in the outer reg ...

...cebound/2017/0217/Hunt-for-Planet-9-how-you-can-help-NASA-search-for-brown-dwarfs-and-low-mass-stars|work=[[The Christian Science Monitor]]|date=17 February ...n the Backyard Worlds: Planet 9 website, here displaying the coldest known brown dwarf [[WISE 0855−0714]] as an orange moving spot in the top left-hand corn ...

...orbit, it is likely to have formed similar to isolated [[Brown dwarf|brown dwarfs]]. It could also have formed in a closer orbit around the star via [[Nebula ....01694 |last1=Phillips |first1=Caprice L. |title=Retrieving Young Cloudy L-Dwarfs: A Nearby Planetary-Mass Companion BD+60 1417B and Its Isolated Red Twin W0 ...

<ref name="Borgniet2017">{{cite journal | title=Extrasolar planets and brown dwarfs around AF-type stars. IX. The HARPS southern sample | url=https://www.aanda ...

| caption1 = Hertzsprung-Russell diagram showing only [[white dwarfs]] with data from ESA's [[Gaia (spacecraft)|Gaia mission]] ...Core crystallization and pile-up in the cooling sequence of evolving white dwarfs|journal=Nature|language=en|volume=565|issue=7738|pages=202–205|doi=10.1038/ ...