Results 1 to 10 of about 37,244 (118)
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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Symposium - International Astronomical Union, 1991 Recent results on low mass AGB stars are presented. Observed amounts of AGB mass loss imply that thermal pulses will only be encountered for stars of initial mass less than about 4M⊙ for Pop I and 3 M⊙ for Pop II. Mc – L, Me – τif, and Mc – Tb relations are summarized.
I.-Juliana Sackmann, Arnold I. Boothroyd
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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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Carbon monoxide in low-mass dwarf stars [PDF]
Monthly Notices of the Royal Astronomical Society, 2005 We compare high resolution infrared observations of the CO 3-1 bands in the 2.297-2.310 micron region of M dwarfs and one L dwarf with theoretical expectations. We find a good match between the observational and synthetic spectra throughout the 2000-3500K temperature regime investigated.
Jones, Hugh R. A. +6 more
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