Circumstellar Molecular Gas Towards L1551-IRS5 and B335

Details Circumstellar Molecular Gas Towards L1551-IRS5 and B335 Circumstellar Molecular Gas Towards L1551-IRS5 and B335

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.260..205w&link_type=abstract

Space-borne Sub-Millimeter Astronomy Mission, Proceedings of an ESA Workshop held in Segovia, Spain, 4-7 Jun. 1986. Edited by N

Astronomy and Astrophysics

Astronomy

Scientific paper

A dense molecular concentration has been detected in the J = 1→0 transition of C18O towards the compact submillimeter sources in L1551 and B 335. The CO/H2 abundance ratio appears normal in L1551 but CO may be depleted by an order of magnitude in B 335. The authors show evidence that high density clumps from the L1551 circumstellar region are being caught up in the CO outflow.

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