The structure of protoplanetary disks surrounding three young intermediate mass stars
The structure of protoplanetary disks surrounding three young intermediate mass stars
We present high-spectral-resolution, optical spectra of three young, intermediate-mass stars, in all of which we spectrally resolve the 6300 Å [OI] emission line. Two of these have a double-peaked line-profile. We attempt to fit these data using a simple model of [OI] emission, which is generated by photo-dissociation of OH …