Results 1 to 10 of about 38,825 (167)
Star Formation as Seen by Low Mass Stars
Acta 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
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TOI-5375 B: A Very Low Mass Star at the Hydrogen-burning Limit Orbiting an Early M-type Star
The 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
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Influence of the initial orbital period and accretion efficiency on the low-mass binary evolution [PDF]
Serbian 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.
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THE MASS-RADIUS(-ROTATION?) RELATION FOR LOW-MASS STARS [PDF]
The Astrophysical Journal, 2011 Accepted to ApJ; 21 pages, 10 figures, 8 tables in emulateapj format.
Kraus, Adam L. +4 more
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Semiconvective mixing in low-mass stars [PDF]
Astrophysics and Space Science, 2010 Conference Proceedings HELAS Workshop on 'Synergies between solar and stellar modelling', Rome, June 2009, Astrophys.
Silva Aguirre, V. +3 more
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Metallicity of low-mass stars in Orion [PDF]
Astronomy & Astrophysics, 2009 13 pages, accepted for publication in A& ...
D'Orazi, V. +5 more
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The empirical mass-luminosity relation for low mass stars [PDF]
Astrophysics 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
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The EBLM Project—From False Positives to Benchmark Stars and Circumbinary Exoplanets
Universe, 2023 The EBLM project aims to characterise very-low-mass stars that are companions to solar-type stars in eclipsing binaries. We describe the history and motivation for this project, the methodology we use to obtain the precise mass, radius, and effective ...
Pierre F. L. Maxted +2 more
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Low-mass relics of early star formation [PDF]
Nature, 2003 Offprint of Nature 422 (2003), 869-871 (issue 24 April 2003)
SCHNEIDER R. +4 more
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Dynamical Masses of Low-mass Stars in the Taurus and Ophiuchus Star-forming Regions [PDF]
The Astrophysical Journal, 2017 Abstract We report new dynamical masses for five pre-main sequence (PMS) stars in the L1495 region of the Taurus star-forming region (SFR) and six in the L1688 region of the Ophiuchus SFR. Since these regions have VLBA parallaxes, these are absolute measurements of the stars’ masses and are independent of their effective temperatures and
Simon, M. +10 more
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