C H A N D R A
S C I E N C E
C E N T E R O B S E R V A T I O N C A T A L O G |
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Abstract: The dwarf carbon stars are a class of post-mass transfer binaries that have accreted a significant amount of C-rich mass and angular momentum from a former AGB companion (now a white dwarf, usually undetected in the optical). We aim to use these dwarf carbon stars to better understand the physics behind mass and angular momentum transfer in binary systems, and the resulting spin-up and activity lifetimes of rejuvenated dwarfs. We propose to use joint Chandra+HST observations of 5 nearby dwarf carbon stars in wide binary systems to (1) probe the dC X-ray magnetic activity and diagnose mass-transfer spin-up, (2) constrain the coronal temperature of the dC, and (3) assess the remnant white dwarf companion cooling age through UV photometry. |
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