A rotating gas disk around L1551 IRS 5?

Details A rotating gas disk around L1551 IRS 5? A rotating gas disk around L1551 IRS 5?

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...298l..19b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 298, Nov. 1, 1985, p. L19, L20.

Astronomy and Astrophysics

Astrophysics

28

Interstellar Matter, Molecular Clouds, Pre-Main Sequence Stars, Rotating Disks, Flow Velocity, Infrared Stars, Stellar Mass Ejection

Scientific paper

The 100 m telescope in Effelsberg equipped with a cooled mixer receiver was used to check the claimed detection of a velocity gradient in the CS 1-0 transition, in a so-called proto-planetary disk around L1551 IRS 5. The authors find no significant velocity gradient. The new data disagree with the model of a rotating disk of interstellar dimensions, which might have played a role in confining the bipolar flow from L1551 IRS 5.

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