Results 91 to 100 of about 553,339 (197)
Linearity of Structure Kernels in Main-sequence and Subgiant Solar-like Oscillators
The Astrophysical JournalSeismic structure inversions have been used to study the solar interior for decades. With the high-precision frequencies obtained using data from the Kepler mission, it has now become possible to study other solar-like oscillators using structure ...
Lynn Buchele +3 more
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Constraining Mass-Loss & Lifetimes of Low Mass, Low Metallicity AGB Stars
, 2014 5 pages, 3 figures, proceedings of the conference "Why Galaxies Care About AGB Stars III", Vienna July 28 - August 1, 2014 to appear in an upcoming ASP Conference Series ...
Rosenfield, Philip +9 more
openaire +2 more sources
New Ultracool Companions to Nearby White Dwarfs
The Astronomical JournalWe conducted a search for new ultracool companions to nearby white dwarfs using multiple methods, including the analysis of colors and examination of images in both the optical and the infrared.
Alexia Bravo +17 more
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Magnetic topologies of cool stars [PDF]
, 2007 Stellar magnetic fields can be investigated using several, very complementary approaches. While conventional spectroscopy is capable of estimating the average magnetic strength of potentially complex field configurations thanks to its low sensitivity to ...
Bouvier, J. +16 more
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Olivier Chesneau's Work on Low Mass Stars [PDF]
EAS Publications Series, 2015 During his too short career, Olivier Chesneau pioneered the study of the circumstellar environments of low mass evolved stars using very high angular resolution techniques. He applied state of the art high angular resolution techniques, such as optical interferometry and adaptive optics imaging, to the the study of a variety of objects, from AGB stars ...
openaire +2 more sources
Demographics of M Dwarf Binary Exoplanet Hosts Discovered by TESS
The Astronomical JournalM dwarfs have become increasingly important in the detection of exoplanets and the study of Earth-sized planets and their habitability. However, 20%–30% of M dwarfs have companions that can impact the formation and evolution of planetary systems.
Rachel A. Matson +17 more
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EPJ Web of Conferences, 2017 We present the first results of a detailed comparison between the pulsation properties of pulsating Extremely Low-Mass pre-white dwarf stars (the pre-ELMV variable stars) and δ Scuti stars.
Arias J.P.Sánchez +3 more
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2D dynamics of the radiative core of low mass stars
EPJ Web of Conferences, 2017 Understanding the internal rotation of low mass stars all along their evolution is of primary interest when studying their rotational dynamics, internal mixing and magnetic field generation.
Hypolite Delphine +2 more
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The Astrophysical JournalRapid rotation and nonradial pulsations enable Be stars to build decretion disks, where the characteristic line emission forms. A major but unconstrained fraction of Be stars owe their rapid rotation to mass and angular momentum transfer in a binary. The
Robert Klement +10 more
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