Constraining the Stellar Mass Function in the Galactic Center via Mass Loss from Stellar Collisions

<table>The fraction of flux emitted from unbound material at radius <svg height="13.3125" id="M336" style="vertical-align:-5.04861pt" version="1.1" viewbox="0 0 20.375 13.3125" width="20.375" xmlns="http://www.w3.org/2000/svg">
<g transform="matrix(1.25,0,0,-1.25,0,13.3125)">
<g transform="translate(72,-61.35)">
<text transform="matrix(1,0,0,-1,-71.95,66.44)">
<tspan style="font-size: 12.50px; " x="0" y="0">𝑟</tspan>
</text>
<text transform="matrix(1,0,0,-1,-66.85,63.31)">
<tspan style="font-size: 8.75px; " x="0" y="0">g</tspan>
<tspan style="font-size: 8.75px; " x="4.2884798" y="0">a</tspan>
<tspan style="font-size: 8.75px; " x="8.1743679" y="0">l</tspan>
</text>
</g>
</g>
</svg> that contributes to the 2–10 keV band.</table>

Advances in Astronomy

fig12

Figure 12

Figure 12: Constraining the Stellar Mass Function in the Galactic Center via Mass Loss from Stellar Collisions 