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Magnetism, dynamo action and the solar-stellar connection
The Sun and other stars are magnetic: magnetism pervades their interiors and affects their
evolution in a variety of ways. In the Sun, both the fields themselves and their influence on …
evolution in a variety of ways. In the Sun, both the fields themselves and their influence on …
Accurate masses and radii of normal stars: modern results and applications
G Torres, J Andersen, A Giménez - The Astronomy and Astrophysics …, 2010 - Springer
This article presents and discusses a critical compilation of accurate, fundamental
determinations of stellar masses and radii. We have identified 95 detached binary systems …
determinations of stellar masses and radii. We have identified 95 detached binary systems …
How to constrain your M dwarf: measuring effective temperature, bolometric luminosity, mass, and radius
Precise and accurate parameters for late-type (late K and M) dwarf stars are important for
characterization of any orbiting planets, but such determinations have been hampered by …
characterization of any orbiting planets, but such determinations have been hampered by …
Magnetic fields of M dwarfs
Magnetic fields play a fundamental role for interior and atmospheric properties of M dwarfs
and greatly influence terrestrial planets orbiting in the habitable zones of these low-mass …
and greatly influence terrestrial planets orbiting in the habitable zones of these low-mass …
Giant planet occurrence in the stellar mass-metallicity plane
Correlations between stellar properties and the occurrence rate of exoplanets can be used
to inform the target selection of future planet-search efforts and provide valuable clues about …
to inform the target selection of future planet-search efforts and provide valuable clues about …
Metallicity and temperature indicators in M dwarf K-band spectra: Testing new and updated calibrations with observations of 133 solar neighborhood M dwarfs
We present K-band spectra for 133 nearby (d< 33 ps) M dwarfs, including 18 M dwarfs with
reliable metallicity estimates (as inferred from an FGK type companion), 11 M dwarf planet …
reliable metallicity estimates (as inferred from an FGK type companion), 11 M dwarf planet …
The habitability of planets orbiting M-dwarf stars
The prospects for the habitability of M-dwarf planets have long been debated, due to key
differences between the unique stellar and planetary environments around these low-mass …
differences between the unique stellar and planetary environments around these low-mass …
Solar-type dynamo behaviour in fully convective stars without a tachocline
In solar-type stars (with radiative cores and convective envelopes like our Sun), the
magnetic field powers star spots, flares and other solar phenomena, as well as …
magnetic field powers star spots, flares and other solar phenomena, as well as …
Testing a predictive theoretical model for the mass loss rates of cool stars
SR Cranmer, SH Saar - The Astrophysical Journal, 2011 - iopscience.iop.org
The basic mechanisms responsible for producing winds from cool, late-type stars are still
largely unknown. We take inspiration from recent progress in understanding solar wind …
largely unknown. We take inspiration from recent progress in understanding solar wind …
The spots models: a grid of theoretical stellar evolution tracks and isochrones for testing the effects of starspots on structure and colors
One-dimensional stellar evolution models have been successful at representing the
structure and evolution of stars in diverse astrophysical contexts, but complications have …
structure and evolution of stars in diverse astrophysical contexts, but complications have …