Depletion of CCS in a Candidate Warm-Carbon-Chain-Chemistry Source L483

Abstract

We have carried out an observation of the CCS ($J_N$=2${}_1-$1${}_0$) line with the Very Large Array in its D-configuration toward a protostellar core L483 (IRAS~18140$-$0440). This is a candidate source of the newly found carbon-chain rich environment called "Warm-Carbon-Chain-Chemistry (WCCC)", according to the previous observations of carbon-chain molecules. The CCS distribution in L483 is found to consist of two clumps aligned in the northwest-southeast direction, well tracing the CCS ridge observed with the single-dish radio telescope. The most remarkable feature is that CCS is depleted at the core center. Such a CCS distribution with the central hole is consistent with those of previously observed prestellar and protostellar cores, but it is rather unexpected for L483. This is because the distribution of CS, which is usually similar to that of CCS, is centrally peaked. Our results imply that the CCS ($J_N$=2${}_1-$1${}_0$) line would selectively trace the outer cold envelope in the chemically less evolved phase that is seriously resolved out with the interferometric observation. Thus, it is most likely that the high abundance of CCS in L483 relative to the other WCCC sources is not due to the activity of the protostar, although it would be related to its younger chemical evolutionary stage, or a short timescale of the prestellar phase.

10 pages, 3 figures, accepted for publication in ApJ Part 1

References in corpus (2)

• Modeling the Lukewarm Corino Phase - is L1527 unique?
• Molecular Line Observations of a Carbon-Chain-Rich Core L492

Cited by in corpus (7)

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• The connection between warm carbon chain chemistry and interstellar irradiation of star-forming cores
• Molecular Distributions of the Disk/Envelope System of L483: Principal Component Analysis for the Image Cube Data
• Chemical evolution of the HC3N and N2H+ molecules in dense cores of the Vela C giant molecular cloud complex
• Detection of Two Carbon-Chain-Rich Cores; CB130-3 and L673-SMM4
• Imaging of the CCS 22.3 GHz emission in the Taurus Molecular Cloud complex