Results 1 to 10 of about 40,072 (165)
Pulsation in extremely low-mass helium stars [PDF]
Monthly Notices of the Royal Astronomical Society, 2013 AbstractWe explore the stability of extremely low-mass stars (M < 0.25 M⊙) across a wide range of composition, effective temperature, and luminosity. We identify the instability boundaries associated with radial oscillations. These are a strong function of both composition and radial order (0 ≤ n ≤ 13).
C. S. Jeffery, Hideyuki Saio
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Measuring the magnetic fields in the chromospheres of low-mass stars. [PDF]
Nat CommunCang T +13 more
europepmc +3 more sources
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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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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Efficiencies of Low‐Mass Star and Star Cluster Formation
The Astrophysical Journal, 2000 20 pages, 2 figures, accepted by ...
Matzner, Christopher D. +1 more
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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 - 4M<sub>ʘ</sub>), metallicities (0:1 - 1 Z<sub>ʘ</sub>) and ages (0:5 - 30 Myr).
Nino Panagia, Guido De Marchi
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Evolution and Nucleosynthesis of Primordial Low‐Mass Stars
The Astrophysical Journal, 2004 We discuss in detail the evolutionary properties of low mass stars M< 1 M(Solar) having metallicity lower than Z=10^(-6) from the pre- main sequence up to (almost) the end of the Asymptotic Giant Branch phase. We also discuss the possibility that the large [C,N/Fe] observed on the surface of the most Iron poor star presently known, HE0107-5240, may ...
I. PICARDI +7 more
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Low-Mass Stars. II. The Core Mass--Luminosity Relations for Low-Mass Stars
The Astrophysical Journal, 1988 Etude de la relation masse-luminosite dans la litterature pour des etoiles de masse intermediaire, et extension a des etoiles de faible masse (0,8 M ○. -3 M ○. )
Arnold I. Boothroyd, I.-Juliana Sackmann
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Rotation of Low-mass Stars in Taurus with K2 [PDF]
The Astronomical Journal, 2020 Abstract We present an analysis of K2 light curves (LCs) from Campaigns 4 and 13 for members of the young (∼3 Myr) Taurus association, in addition to an older (∼30 Myr) population of stars that is largely in the foreground of the Taurus molecular clouds.
L. M. Rebull +6 more
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