Results 181 to 190 of about 173,010 (211)
Diagnostics of Stellar Chromospheres and Transition Regions
A. C. Lanzafame
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Science (New York, N.Y.), 2010
Besides being of intrinsic interest, these outer stellar envelopes provide very useful astrophysical tools. ; © 1966 American Association for the Advancement of Science.
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Besides being of intrinsic interest, these outer stellar envelopes provide very useful astrophysical tools. ; © 1966 American Association for the Advancement of Science.
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Chromospheric Lines as Diagnostics of Stellar Oscillations
2008Gravitational waves in the chromosphere, theorized as early as 1963 [10], are thoroughly explored in the more recent papers by [7, 8]. Theory predicts that the convective overshoot in the upper photosphere and low chromosphere will readily excite gravity waves.
Diane B. Paulson +6 more
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Stellar chromospheres and coronae in the Ursa Major Cluster stars
, 1984F. Walter +4 more
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Heating of stellar chromospheres and coronae observational constraints and evidence for saturation
, 1987O. Vilhu
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Stellar chromospheric activity in main-sequence stars
The research presented here presents a narrow slice of several largescale, ground-based astronomy surveys focused on chromospheric activity measurements of stars from the Keck Observatory. We conducted a comprehensive study analyzing chromospheric activity and its relationship with stellar properties in exoplanet host stars and solar neighborhood stars.openaire +1 more source
The boundary line in the H-R diagram for stellar chromospheres and the theory of convection
, 1980E. Boehm-Vitense, T. Dettmann
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Philosophical transactions of the Royal Society of London. Series A: Mathematical and physical sciences, 1971
H. Zirin
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H. Zirin
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Heating of stellar chromospheres and coronae: Evidence for non-magnetic heating
, 1987C. Schrijver
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