The stellar content of obscured galactic giant HII regions. III. W31

We present near-infrared (J, H, and K) photometry and moderate-resolution ( lambda/Delta lambda =3000) K-band spectroscopy of the embedded stellar clus ter in the giant H II region W31. Four of the brightest five cluster member s are early O-type stars based on their spectra. We derive a spectrophotome tric distance for W31 of 3.4 +/-0.3 kpc using these new spectral types and infrared photometry. The brightest cluster source at K is a red object that lies in the region of the J-H versus H-K color-color plot inhabited by sta rs with excess emission in the K band. This point source has an H- plus K-b and spectrum that shows no photospheric features, which we interpret as bei ng the result of veiling by local dust emission. Strong Brackett series emi ssion and permitted Fe II emission are detected in this source; the latter feature is suggestive of a dense inflow or outflow. The near-infrared posit ion of this red source is consistent with the position of a 5 GHz thermal r adio source seen in previous high angular resolution VLA images. We also id entify several other K-band sources containing excess emission with compact radio sources. These objects may represent stars in the W31 cluster still embedded in their birth cocoons.