Abstract
view Abstract Citations (41) References (27) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Properties of the chromosphere-corona transition region in Capella. Haisch, B. M. ; Linsky, J. L. Abstract Analysis of recent ultraviolet observations of the Capella binary system (Alpha Aur) indicates a dense geometrically narrow chromosphere-corona transition region in the Capella system primary (G5 III) similar in many respects to a solar active region. An examination of the coronal energy balance, together with the coronal base pressure derived from the line fluxes, predicts a corona with a mean temperature of 1.2 million K and a large stellar wind consistent with observations. Publication: The Astrophysical Journal Pub Date: April 1976 DOI: 10.1086/182085 Bibcode: 1976ApJ...205L..39H Keywords: Binary Stars; Chromosphere; Coronas; Late Stars; Stellar Spectra; Ultraviolet Spectra; Astronomical Spectroscopy; Line Spectra; Solar Activity; Stellar Mass; Stellar Winds; Astrophysics full text sources ADS |
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