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High Resolution X-Ray Spectra of Capella: Initial Results from the Chandra High Energy Transmission Grating Spectrometer

C. R. Canizares·D. P. Huenemoerder·D. S. Davis·D. Dewey·K. A. Flanagan·J. Houck·T. H. Markert·H. L. Marshall·M. L. Schattenburg·N. S. Schulz·M. Wise·J. J. Drake·N. S. Brickhouse
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Abstract

High resolution spectra of the active binary Capella (G8 III + G1 III) covering the energy range 0.4-8.0 keV (1.5-30 Angstroms) show a large number of emission lines, demonstrating the performance of the HETGS. A preliminary application of plasma diagnostics provides information on coronal temperatures and densities. Lines arising from different elements in a range of ionization states indicate that Capella has plasma with a broad range of temperatures, from log T = 6.3 to 7.2, generally consistent with recent results from observations with the Extreme Ultraviolet Explorer (EUVE) and the Advanced Satellite for Cosmology and Astrophysics (ASCA). The electron density is determined from He-like O VII lines, giving the value N_e=10^10 cm^-3 at T_e=2*10^6 K; He-like lines formed at higher temperatures give only upper limits to the electron density. The density and emission measure from O VII lines together indicate that the coronal loops are significantly smaller than the stellar radius.

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C. R. Canizares, D. P. Huenemoerder, D. S. Davis, D. Dewey, K. A. Flanagan, J. Houck, T. H. Markert, H. L. Marshall, M. L. Schattenburg, N. S. Schulz, M. Wise, J. J. Drake, N. S. Brickhouse. 2000-06-30. High Resolution X-Ray Spectra of Capella: Initial Results from the Chandra High Energy Transmission Grating Spectrometer. https://doi.org/10.1086/312823

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