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Accurate geometric albedo, shape, and size of Hi'iaka from a stellar occultation. [PDF]
Fernández-Valenzuela E +73 more
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Food deprivation is associated with telomere elongation during hibernation in a primate. [PDF]
Blanco MB +4 more
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Precise Masses Reveal that TOI-700 c is Low Density and TOI-700 d is Rocky
Gilbert E +35 more
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Radial velocities of M dwarf stars
Publications of the Astronomical Society of the Pacific, 1987Radial velocities for 72 M dwarfs have been obtained having internal errors of about 0.1 km/s and external errors of about 0.4 km/s. Multiple velocity measurements of ten dMe stars have yielded a set of six which have no stellar companions, providing confirmation that the dMe phenomenon can occur in single stars.
Geoffrey W. Marcy +2 more
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Coronal Structure in M Dwarf Stars
1996In view of the importance of these objects as observational probes for theories of stellar dynamos and coronal heating, as well as their potentially important role in the galactic environment, we implemented a program of pointed ROSAT PSPC observations of selected M dwarfs in the solar neighborhood.
M. S. Giampapa +5 more
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Photometry of Dwarf K and M Stars
Publications of the Astronomical Society of the Pacific, 1988Broad-band UBVRI photometry is presented for 50 dwarf K and M stars, most without previou photometry, from the lists of Vyssotsky.
John Booth, Joseph Caruso, E. W. Weis
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The Internal Structure of M Dwarf Stars
Publications of the Astronomical Society of Japan, 1960Abstract Models for M dwarfs which consist of a convective envelope and a radiative core are computed with the effects of electron degeneracy taken into account. The results show that in the middle M dwarf, such as Krüger 60A, O2 Eri C and Krüger 60B, the convective envelope extends inward attaining to more than 40% of the stellar radius
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Abundance Survey of M and K Dwarf Stars
Nuclear Physics A, 2005We report the measurement of chemical abundances in 35 low-mass main sequence (M and K dwarf) stars. We have measured the abundance of 12 elements in Kapteyn's Star, a nearby halo M subdwarf. The abundances indicate an iron abundance of [Fe/H] = −0.98, which is about 0.5 dex smaller than that measured in the only previous published measurement using ...
Vincent M. Woolf, George Wallerstein
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