A Cyanopolyyne-rich but Complex-organic-molecule-poor Massive Protostar: The First Hot Carbon-chain Chemistry Source G28.28-0.36

Abstract We present molecular emission line data from the massive young stellar object (MYSO) G28.28-0.36 (G28.28) obtained with the Atacama Large Millimeter/submillimeter Array Band 3. Cyanopolyynes (HC 3 N and HC 5 N) and three complex organic molecules (COMs; CH 3 OH, CH 3 CN, and CH 3 CHO) are detected from the MYSO G28.28. In addition, strong emission regions of cyanopolyynes are identified between G28.28 and a nearby ultracompact H ii region. The HC 5 N emission is coincident with the dust continuum peak, where an excitation temperature of 100 K is derived from CH 3 CN. These results suggest that the hot carbon-chain chemistry (HCCC) mechanism produces cyanopolyynes in the hot region around G28.28. We find that G28.28 exhibits a unique chemical feature: cyanopolyynes are abundant, but COMs are deficient, unlike the other MYSOs studied previously. These results imply that G28.28 is a counterpart of the warm carbon-chain chemistry (WCCC) low-mass source L1527. G28.28 is the first HCCC source identified so far.

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Journal
The Astrophysical Journal
Published
2026-11-02
DOI
https://doi.org/10.3847/1538-4357/aeacdb
Primary Topic
Astrophysics and Star Formation Studies
Type
article
Field-Weighted Citation Impact
0.00

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article

A Cyanopolyyne-rich but Complex-organic-molecule-poor Massive Protostar: The First Hot Carbon-chain Chemistry Source G28.28-0.36

Prasanta Gorai, Tomomi Shimoikura, Kazuhito Dobashi, O. Sipilä et al.
The Astrophysical Journal
Astrophysics and Star Formation Studies
article

A Cyanopolyyne-rich but Complex-organic-molecule-poor Massive Protostar: The First Hot Carbon-chain Chemistry Source G28.28-0.36

Prasanta Gorai, Tomomi Shimoikura, Kazuhito Dobashi, O. Sipilä, T. K. Sridharan, Kotomi Taniguchi, Masao Saito, Paola Caselli, Jonathan C. Tan
article en

Abstract

Abstract We present molecular emission line data from the massive young stellar object (MYSO) G28.28-0.36 (G28.28) obtained with the Atacama Large Millimeter/submillimeter Array Band 3. Cyanopolyynes (HC 3 N and HC 5 N) and three complex organic molecules (COMs; CH 3 OH, CH 3 CN, and CH 3 CHO) are detected from the MYSO G28.28. In addition, strong emission regions of cyanopolyynes are identified between G28.28 and a nearby ultracompact H ii region. The HC 5 N emission is coincident with the dust continuum peak, where an excitation temperature of 100 K is derived from CH 3 CN. These results suggest that the hot carbon-chain chemistry (HCCC) mechanism produces cyanopolyynes in the hot region around G28.28. We find that G28.28 exhibits a unique chemical feature: cyanopolyynes are abundant, but COMs are deficient, unlike the other MYSOs studied previously. These results imply that G28.28 is a counterpart of the warm carbon-chain chemistry (WCCC) low-mass source L1527. G28.28 is the first HCCC source identified so far.

The Astrophysical JournalVol. 1011(2)
Otsuma Women's University (JP), Tokyo Gakugei University (JP), University of Oslo (NO), National Institutes of Natural Sciences (JP), The Graduate University for Advanced Studies, SOKENDAI (JP), Heidelberg University (DE), National Radio Astronomy Observatory (US), Max Planck Institute for Extraterrestrial Physics (DE), University of Virginia (US), Chalmers University of Technology (SE)
National Science Foundation, National Radio Astronomy Observatory, Korea Astronomy and Space Science Institute, Max-Planck-Gesellschaft, National Astronomical Observatory of Japan, National Science and Technology Council, Japan Society for the Promotion of Science, National Institutes of Natural Sciences
Openalex Percentile: Top 27%
Astrophysics and Star Formation Studies
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