BIMA observations of infall in L1544: a young starless core in Taurus

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Scientific paper

We present high resolution observations of n2hp(1-0) in the starless, dense core L1544 in Taurus made with the BIMA interferometer. Red-shifted self-absorption, indicative of inward motions, is found toward the center of an elongated core. The data are fit by a non-spherical model consisting of two isothermal, rotating, centrally condensed layers. Through a hybrid global-individual fit to the spectra, we map the variation of infall speed at scales ~1400 AU and find values ~0.08 kms around the core center. The inward motions are small in comparison to thermal, rotational, and gravitational speeds but are large enough to suggest that L1544 is very close to forming a star.

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