Infrared spectroscopy of symbiotic stars. IX. d-type symbiotic novae
Time-series spectra of the near-infrared 1.6 μm region have been obtained for five of the six known D-type symbiotic novae. The spectra map the pulsation kinematics of the Mira component in the Mira-white dwarf binary system and provide the center-of-mas
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|Source:||Astrophysical Journal, The|
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