Very Large Array observations of the Galactic Center at 7 mm have produced an image of the 30 ^ { \prime \prime } surrounding Sgr A * with a resolution of \sim 82 \times 42 milliarcseconds ( mas ) .
A comparison with IR images taken simultaneously with the Very Large Telescope ( VLT ) identifies 41 radio sources with L-band ( 3.8 \mu m ) stellar counterparts .
The well-known young , massive stars in the central Sgr A * cluster ( e.g. , IRS 16C , IRS 16NE , IRS 16SE2 , IRS 16NW , IRS 16SW , AF , AFNW , IRS 34W and IRS 33E ) are detected with peak flux densities between \sim 0.2 and 1.3 mJy .
The origin of the stellar radio emission in the central cluster is discussed in terms of ionized stellar winds with mass-loss rates in the range \sim 0.8 - 5 \times 10 ^ { -5 } M _ { \odot } yr ^ { -1 } .
Radio emission from eight massive stars is used as a tool for registration between the radio and infrared frames with mas precision within a few arcseconds of Sgr A * .
This is similar to the established technique of aligning SiO masers and evolved stars except that radio stars lie within a few arcseconds of Sgr A* .
Our data show a scatter of \sim 6.5 mas in the positions of the eight radio sources that appear in both the L-band and 7 mm images .
Lastly , we use the radio and IR data to argue that members of IRS 13N are Young Stellar Objects rather than dust clumps , supporting the hypothesis that recent star formation has occurred near Sgr A* .