Ab initio studies on the interstellar molecules C3H2 and C3H and the mechanism for the neutral-neutral reaction C(3 P)+C2H2We studied the structure of disiloxane ͑H 3 Si-O-SiH 3 ͒, silanol ͑H 3 Si-OH͒, and the silanol anion ͑H 3 Si-O Ϫ ͒ with ab initio molecular orbital theory and the correlation consistent polarized basis sets of Dunning and co-workers. We present results for the correlation consistent polarized valence double zeta ͑cc-pVDZ͒, triple zeta ͑cc-pVTZ͒, and quadruple zeta ͓cc-pVQZ͑-g͔͒ basis sets. Optimized geometries and energies are given at both the restricted Hartree-Fock ͑RHF͒ level and with the inclusion of electron correlation by second order Mo "ller-Plesset perturbation theory ͑MP2͒. The correlation consistent basis sets provide a systematic expansion of the orbital basis set, with each set of additional functions adding a similar contribution to the correlation energy. We find that the calculated molecular properties show exponential convergence with increasing basis set size. These calculations answer long-standing questions regarding the structure and barrier to linearization of disiloxane. Results at the highest level of theory ͓MP2/cc-pVQZ͑-g͔͒ for disiloxane gave a Si-O-Si bond angle of 147.0°, a Si-O bond length of 1.641 Å, and a barrier to linearization of 0.4 kcal/mol. All of these values are in excellent agreement with experimental results. Similar calculations for silanol gave a Si-O bond length of 1.655 Å, an O-H bond of 0.955 Å, and a Si-O-H angle of 117.9°. The MP2/cc-pVQZ͑-g͒ deprotonation energy ͑⌬E 0 ͒ for silanol, calculated as the energy difference between silanol and its anion, is Ϫ366.6 kcal/mol. The effects of electron correlation at the MP4 level are studied in all three molecules using the cc-pVDZ and cc-pVTZ basis sets.