Results 11 to 20 of about 11,210,903 (298)
Star Formation as Seen by Low Mass Stars
Using the Hubble Space Telescope (HST) we have characterised and compared the physical properties of a large sample of pre-main sequence (PMS) stars spanning a wide range of masses (0:5 - 4Mʘ), metallicities (0:1 - 1 Zʘ) and ages (0:5 - 30 Myr).
Nino Panagia, Guido De Marchi
doaj +2 more sources
Models of very-low-mass stars, brown dwarfs and exoplanets. [PDF]
Allard F, Homeier D, Freytag B.
europepmc +2 more sources
Three low-mass companions around aged stars discovered by TESS [PDF]
We report the discovery of three transiting low-mass companions to aged stars: a brown dwarf (TOI-2336b) and two objects near the hydrogen burning mass limit (TOI-1608b and TOI-2521b).
Paegert, Martin +109 more
core +1 more source
TOI-5375 B: A Very Low Mass Star at the Hydrogen-burning Limit Orbiting an Early M-type Star
The Transiting Exoplanet Survey Satellite (TESS) mission detected a companion orbiting TIC 71268730, categorized it as a planet candidate, and designated the system TOI-5375.
Mika Lambert +18 more
doaj +1 more source
THE MASS-RADIUS(-ROTATION?) RELATION FOR LOW-MASS STARS [PDF]
Accepted to ApJ; 21 pages, 10 figures, 8 tables in emulateapj format.
Kraus, Adam L. +4 more
openaire +3 more sources
TOI 694b and TIC 220568520b: Two Low-mass Companions near the Hydrogen-burning Mass Limit Orbiting Sun-like Stars [PDF]
We report the discovery of TOI 694 b and TIC 220568520 b, two low-mass stellar companions in eccentric orbits around metal-rich Sun-like stars, first detected by the Transiting Exoplanet Survey Satellite (TESS).
Flowers, Erin +42 more
core +1 more source
Semiconvective mixing in low-mass stars [PDF]
Conference Proceedings HELAS Workshop on 'Synergies between solar and stellar modelling', Rome, June 2009, Astrophys.
Silva Aguirre, V. +3 more
openaire +4 more sources
Influence of the initial orbital period and accretion efficiency on the low-mass binary evolution [PDF]
This paper presents detailed evolutionary models of low-mass binary systems (1.25 + 1 M⊙) with initial orbital periods of 10, 50 and 100 days and accretion efficiency of 10%, 20%, 50%, and a conservative assumption.
Petrović J.
doaj +1 more source
Metallicity of low-mass stars in Orion [PDF]
13 pages, accepted for publication in A& ...
D'Orazi, V. +5 more
openaire +3 more sources
The empirical mass-luminosity relation for low mass stars [PDF]
This work is devoted to improving empirical mass-luminosity relations and mass-metallicity-luminosity relation for low mass stars. For these stars, observational data in the mass-luminosity plane or the mass-metallicity-luminosity space subject to non-negligible errors in all coordinates with different dimensions.
Xia, Fang, Ren, Shulin, Fu, Yanning
openaire +2 more sources

