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{{Short description|Cluster of stars around a supermassive black hole}} ...black hole]] that has been ejected from the center of its host [[galaxy]]. Stars that are close to the black hole at the time of the ejection will remain bo ...

...le surface conditions.<ref name="Armstrong">{{cite journal |title=The host stars of Kepler's habitable exoplanets: superflares, rotation and activity |autho {{Portal bar|Earth sciences|Astronomy|Stars|Spaceflight|Outer space|Solar System}} ...

...ast6=Levin |first6=Yuri |year=2024 |title=Eddington Envelopes: The Fate of Stars on Parabolic Orbits Tidally Disrupted by Supermassive Black Holes |journal= ...first4=Scott C. |date=2020-12-01 |title=Tidal Disruptions of Main-sequence Stars. III. Stellar Mass Dependence of the Character of Partial Disruptions |jour ...

| variable = [[flare star]]<ref name="Eriksson2020"/> ...12-14 Jupiter-mass object orbiting a young binary system of very low-mass stars |journal=Astronomy and Astrophysics |volume=553 |pages=L5 |doi=10.1051/0004 ...

...million years. Several examples of such disks have been observed to orbit stars with spectral types of [[M-type star|M]] or later. The presence of gas aro ...web|url=https://www.nhn.ou.edu/~smsilver/PeterPanDisks.html|title=Low-mass Stars {{!}} Steven M. Silverberg|website=www.nhn.ou.edu|access-date=2019-07-25}}< ...

...the same processes that lead to other forms of solar activity like [[solar flare]]s and [[coronal mass ejection]]s. ...Dulk|first=George A.|date=1985-09-01|title=Radio Emission from the Sun and Stars|url=https://www.annualreviews.org/doi/10.1146/annurev.aa.23.090185.001125|j ...

| Design = A large golden star within an arc of four smaller golden stars, in the canton, on a field of [[Chinese red]]. ...g elements|canton]]. The design features one large star, with four smaller stars in an arc set off towards the fly. It has been the national flag of China s ...

The most effusive [[solar flare]]s emit across the entire EM spectrum, including γ-rays. The first confiden ...ticle beams is another possible mechanism of gamma ray production. Neutron stars with a very high magnetic field ([[magnetar]]s), thought to produce astrono ...

...[[Astrophysical plasma]]s are also observed in [[accretion disk]]s around stars or compact objects like [[white dwarf]]s, [[neutron star]]s, or [[black hol ...16/S0275-1062(02)00095-4 | title = A rope-shaped solar filament and a IIIb flare | journal = Chinese Astronomy and Astrophysics | volume = 26 | issue = 4 | ...

...]] and [[brown dwarfs]] which are the least voluminous known (the smallest stars by volume). ===Notable small stars=== ...

...t1=Jie-Shuang |title=Fast Radio Bursts from the Inspiral of Double Neutron Stars |last2=Yang |first2=Yuan-Pei |last3=Wu |first3=Xue-Feng |last4=Dai |first4= ...m|last2=Ott|first2=Christian|title=Dark Matter-induced Collapse of Neutron Stars: A Possible Link Between Fast Radio Bursts and the Missing Pulsar Problem|j ...

Below there are lists the nearest stars separated by [[spectral type]]. The scope of the list is still restricted t == List of nearest M-type stars == ...

...TRAPPIST is used to find [[exoplanet]]s, and is preferentially employed on stars colder than {{cvt|3000|K}}.{{sfn|Shields|Ballard|Johnson|2016|p=7}} }} proj ...motion]]{{efn|The movement of the star in the sky, relative to background stars.{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Proper Motion}}}}{{sfn|How ...