Abstract
Herbig Ae/Be objects, like their lower mass counterparts T Tauri stars, are seen to form a stable circumstellar disk which is initially gas-rich and could ultimately form a planetary system. We present Herschel SPIRE 460-1540 GHz spectra of five targets out of a sample of 13 young disk sources, showing line detections mainly due to warm CO gas. Copyright © 2013, International Astronomical Union.
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CITATION STYLE
Van Der Wiel, M. H. D., Naylor, D. A., Aresu, G., & Olofsson, G. (2013). Gas signatures of Herbig Ae/Be disks probed with Herschel SPIRE spectroscopy. In Proceedings of the International Astronomical Union (Vol. 8, pp. 175–176). Cambridge University Press. https://doi.org/10.1017/S1743921313008272
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