What is the reason for the lack of cool evolved stars near the center of the Galaxy?

Abstract

The observed deficit of bright late-type giants in the central parsec of the Milky Way remains an open problem. We investigate whether repeated passages of red giants (RGs) through a past jet from Sgr A${}^{\ast }$ can modify their envelopes and apparent spectral types. Three-dimensional hydrodynamical simulations follow a $1M_{\odot }$, $100R_{\odot }$ RG through up to ten jet crossings at $10^{-3}\text{pc}$, using jet kinetic luminosities of $10^{42}$, $10^{44}$, and $10^{48}\text{erg}{\text{s}}^{-1}$. Each passage produces shocks, envelope ablation, and an asymmetric downstream tail. For jet luminosities up to $10^{44}\text{erg}{\text{s}}^{-1}$, the cumulative ablated mass evolves approximately as $\Delta M\propto t^{1/2}$ and reaches about $10^{-4}{M}_{\odot }$ over a $10^5\text{yr}$ active phase. Repeated heating also raises the surface temperature from about $3600$ to $8500\text{K}$ during the first ten passages, potentially making an M-type giant appear as an A-type source. Jet feedback may therefore contribute to the apparent depletion of cool giants and the excess of hot stars in galactic nuclei (GN).

Proceedings IAU Symposium No. 405: Traversing the Galactic Center in Space and Time