CS observations of L1551 - No rotating disk

Details CS observations of L1551 - No rotating disk CS observations of L1551 - No rotating disk

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...317l..95m&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 317, June 15, 1987, p. L95-L99.

Astronomy and Astrophysics

Astrophysics

30

Carbon Compounds, Interstellar Matter, Molecular Clouds, Pre-Main Sequence Stars, Sulfides, Angular Resolution, Astronomical Maps, Emission Spectra

Scientific paper

High angular resolution observations were made of the CS emission from the core of the L1551 molecular cloud, using a technique of heavy oversampling and maximum entropy reconstruction. These observations are consistent with the data published by Kaifu et al. in 1984 and Batrla and Menten in 1985, but show no evidence for a large rotating molecular disk as proposed by Kaifu et al. The chaotic morphology and kinematics are more suggestive of the disruption of the dense core by the collimated winds from IRS 5.

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