The κ Andromedae system: New constraints on the companion mass, system age, and further multiplicity
κ Andromedae is a B9IVn star at 52 pc for which a faint substellar companion separated by 55 ± 2 AU was recently announced. In this work, we present the first spectrum of the companion, "κ And B," using the Project 1640 high-contrast imaging platform.
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Hinkley_The_κ_Andromedae_system:_New_2013.pdf||1.21 MB||Adobe PDF|
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