Are Giant Planets Forming around HR 4796A?

We have obtained Far Ultraviolet Spectroscopic Explorer and Hubble Space Telescope STIS spectra of HR 4796A, a nearby 8 Myr old main-sequence star that possesses a dusty circumstellar disk whose inclination has been constrained from high-resolution near-infrared observations to be ~17° from edge-on. We searched for circumstellar absorption in the ground states of C II λ1036.3, O I λ1039.2, Zn II λ2026.1, Lyman series H 2 , and CO (A-X) and failed to detect any of these species. We place upper limits on the column densities and infer upper limits on the gas masses assuming that the gas is in hydrostatic equilibrium, is well mixed, and has a temperature T gas ~ 65 K. Our measurements suggest that this system possesses very little molecular gas. Therefore, we infer an upper limit for the gas-to-dust ratio (≤4.0) assuming that the gas is atomic. We measure less gas in this system than is required to form the envelope of Jupiter.