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Herbig Ae/Be objects, like their lower mass counterparts T Tauri stars, areseen to form a stable circumstellar disk which is initially gas-rich and couldultimately form a planetary system. We present Herschel SPIRE 460-1540 GHzspectra of five targets out of a sample of 13 young disk sources, showing linedetections mainly due to warm CO gas.

Gas signatures of Herbig Ae/Be disks probed with Herschel SPIRE spectroscopy