Abstract
We present evidence of a short-lived, transitional stage between the fully embedded and optically visible stages of low-mass star formation. This stage is characterized by a large (2000 AU radius) disk with close-to Keplerian motions, but with a significant inward component to the velocity field. Millimeter-interferometric observations of HCO+ J=1−0 and 3-2 first identified this structure around the embedded object L1489 IRS, with inward motions present on scales of several hundred AU. Subsequent R ≈ 25, 000 M-band spectroscopy showed that the inward motions extend to within 0.1 AU from the star. We conclude that angular-momentum transfer is crucial in determining the final density distribution in the disk and the initial conditions for planet formation.
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Hogerheijde, M.R., Boogert, A.C.A., van Dishoeck, E.F., Blake, G.A. (2002). From Infall to Rotation Around Young Stellar Objects. In: Alves, J.F., McCaughrean, M.J. (eds) The Origins of Stars and Planets: The VLT View. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-40277-1_6
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DOI: https://doi.org/10.1007/978-3-662-40277-1_6
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