Draft:TMTS J0526+5934

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Last edited by 65.92.247.66 (talk | contribs) 2 months ago. (Update)

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TMTS J052610.43+593445.1 (shortened: "TMTS J0526+5934", "TMTS J0526+59") is a binary star system, composed of a white dwarf star (WD) being the "A" element and a B-type hot subdwarf star (sdB) being the "B" element. TMTS J0526+5934 B, the subdwarf, is the smallest known star by volume known of a living fusor, actively fusing star, and the star system has the small period current known, of 20 minutes; both as of 2024. The star system was discovered with the Tsinghua University–Ma Huateng Telescopes for Survey (TMTS)

v t e White dwarf
Formation	Chandrasekhar limit PG 1159 star Stellar evolution Hertzsprung–Russell diagram Mira variable
Fate	Black dwarf Type Ia supernova Candidates Neutron star Pulsar Magnetar Related links Stellar black hole Related links Compact star Quark star Exotic star Extreme helium star Subdwarf B star Helium planet
In binary systems	Nova Remnant List Dwarf nova Micronova Symbiotic nova Cataclysmic variable star AM CVn star Polar Intermediate polar X-ray binary Super soft X-ray source Binary pulsar Helium flash Carbon detonation
Properties	Pulsating Urca process Electron-degenerate matter Quasi-periodic oscillations
Related	Planetary nebula List RAMBOs White dwarf luminosity function Timeline of white dwarfs, neutron stars, and supernovae
List Category

Draft:TMTS J0526+5934

Star system TMTS J0526+59[edit]

White dwarf TMTS J0526+59 A[edit]

Hot subdwarf TMTS J0526+59 B[edit]

References[edit]

See also[edit]