Articles with "dwarf stars" as a keyword



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Properties of Radiative Shock Waves in the Atmospheres of Red Dwarf Stars

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Published in 2019 at "Astrophysics"

DOI: 10.1007/s10511-019-09577-4

Abstract: The emission from the gas behind the front of a stationary shock wave is calculated for the conditions in the atmospheres of red dwarf stars for velocities u0 from 30 to 100 km/s. Energy exchange… read more here.

Keywords: atmospheres red; red dwarf; emission; dwarf stars ... See more keywords
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Why do we find ourselves around a yellow star instead of a red star?

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Published in 2017 at "International Journal of Astrobiology"

DOI: 10.1017/s1473550417000118

Abstract: Abstract M-dwarf stars are more abundant than G-dwarf stars, so our position as observers on a planet orbiting a G-dwarf raises questions about the suitability of other stellar types for supporting life. If we consider… read more here.

Keywords: dwarf stars; around yellow; find around; dwarf ... See more keywords
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Time evolution of rotating and magnetized white dwarf stars

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Published in 2019 at "Monthly Notices of the Royal Astronomical Society"

DOI: 10.1093/mnras/stz1394

Abstract: We investigate the evolution of isolated, zero and finite temperature, massive, uniformly rotating and highly magnetized white dwarf stars under angular momentum loss driven by magnetic dipole braking. We consider the structure and thermal evolution… read more here.

Keywords: evolution; dwarf stars; time; white dwarf ... See more keywords
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Density, not radius, separates rocky and water-rich small planets orbiting M dwarf stars

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Published in 2022 at "Science"

DOI: 10.1126/science.abl7164

Abstract: Exoplanets smaller than Neptune are common around red dwarf stars (M dwarfs), with those that transit their host star constituting the bulk of known temperate worlds amenable for atmospheric characterization. We analyze the masses and… read more here.

Keywords: rocky water; water; separates rocky; water rich ... See more keywords
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The Quest for Pulsating M Dwarf Stars

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Published in 2019 at "Frontiers in Astronomy and Space Sciences"

DOI: 10.3389/fspas.2019.00076

Abstract: Recent fully non-adiabatic theoretical studies of M dwarf models show that they have the potential to excite radial\textbf{,} and low-order, low-degree non-radial modes, as well as solar-like oscillations, due to models being completely convective or… read more here.

Keywords: quest pulsating; pulsating dwarf; dwarf stars; spectroscopy ... See more keywords