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We have conducted a high-dispersion ($R \sim$ 34,000) optical spectroscopicstudy of 10 young stars near the cometary gloule CG 30 in the Gum Nebula, adiffuse H \textsc{ii} region home to at least 32 cometary globules. All 10spectroscopically observed stars at the nebula's northern edge are of low mass(spectral types M4.5 - K5), have broad H$\alpha$ emission, and show spectralveiling. Eight of the 10 are classical T Tauri stars. We spectroscopicallymeasure the photospheric properties of CG 30 IRS 4 inside CG 30. Thoughembedded, CG 30 IRS 4 is T Tauri-like, with relatively slow projected rotationand moderate veiling. Undepleted Li absorptions, strong H$\alpha$ emissions,and positions well above the main sequence on an HR diagram suggest the 10stars are $\lesssim$1 Myr old. Using our measurements, previous spectroscopy,and previous photometry of 11 other young stars in the area, we determinestellar, kinematic, and accretion properties of a total of 21 young stars.Shared radial velocities, proper motions, distances, and ages suggest 14 of theyoung stars (including CG 30 IRS 4) are kinematically related to CG 30. From\textit{Gaia} DR2 distances to 6 of these stars, we derive a distance of$358.1\pm2.2$ pc to the cometary globule complex CG 30/31/38. The CG 30association has an accretor fraction of $29\pm14$\%, low for quiescent clustersof similar age but consistent with other irradiated clusters. The Gum Nebula'smoderate radiation environment ($G_0=6.6^{+3.2}_{-2.7}$ at CG 30) may be strongenough to shorten disk lifetimes.

Young Stars near Cometary Globule CG 30 in the Tumultuous Gum Nebula