Results 11 to 20 of about 11,210,903 (298)

Star Formation as Seen by Low Mass Stars

open access: yesActa Polytechnica CTU Proceedings, 2014
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]

open access: yesPhilos Trans A Math Phys Eng Sci, 2012
Allard F, Homeier D, Freytag B.
europepmc   +2 more sources

Three low-mass companions around aged stars discovered by TESS [PDF]

open access: yes, 2023
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

open access: yesThe Astronomical Journal, 2023
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]

open access: yesThe Astrophysical Journal, 2011
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]

open access: yes, 2020
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]

open access: yesAstrophysics and Space Science, 2010
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]

open access: yesSerbian Astronomical Journal, 2021
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]

open access: yesAstronomy & Astrophysics, 2009
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]

open access: yesAstrophysics and Space Science, 2008
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

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