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位于TMC-1氰基多炔峰处含O的复杂有机分子:CHCHO、CHOH、HCOOCH和CHOCH的检测

O-bearing complex organic molecules at the cyanopolyyne peak of TMC-1: detection of CHCHO, CHOH, HCOOCH, and CHOCH.

作者信息

Agúndez M, Marcelino N, Tercero B, Cabezas C, de Vicente P, Cernicharo J

机构信息

Instituto de Física Fundamental, CSIC, Calle Serrano 123, E-28006 Madrid, Spain.

Observatorio Astronómico Nacional, IGN, Calle Alfonso XII 3, E-28014 Madrid, Spain.

出版信息

Astron Astrophys. 2021 May 5;649. doi: 10.1051/0004-6361/202140978. eCollection 2021 May.

Abstract

We report the detection of the oxygen-bearing complex organic molecules propenal (CHCHO), vinyl alcohol (CHOH), methyl formate (HCOOCH), and dimethyl ether (CHOCH) toward the cyanopolyyne peak of the starless core TMC-1. These molecules are detected through several emission lines in a deep Q-band line survey of TMC-1 carried out with the Yebes 40m telescope. These observations reveal that the cyanopolyyne peak of TMC-1, which is the prototype of cold dark cloud rich in carbon chains, contains also O-bearing complex organic molecules like HCOOCH and CHOCH, which have been previously seen in a handful of cold interstellar clouds. In addition, this is the first secure detection of CHOH in space and the first time that CHCHO and CHOH are detected in a cold environment, adding new pieces in the puzzle of complex organic molecules in cold sources. We derive column densities of (2.2 ± 0.3) × 10 cm, (2.5 ± 0.5) × 10 cm, (1.1 ± 0.2) × 10 cm, and (2.5 ± 0.7) × 10 cm for CHCHO, CHOH, HCOOCH, and CHOCH, respectively. Interestingly, CHOH has an abundance similar to that of its well known isomer acetaldehyde (CHCHO), with CHOH/CHCHO ~ 1 at the cyanopolyyne peak. We discuss potential formation routes to these molecules and recognize that further experimental, theoretical, and astronomical studies are needed to elucidate the true mechanism of formation of these O-bearing complex organic molecules in cold interstellar sources.

摘要

我们报告了在无恒星核心TMC-1的氰基多炔峰处检测到含氧化合物的复杂有机分子丙烯醛(CHCHO)、乙烯醇(CHOH)、甲酸甲酯(HCOOCH)和二甲醚(CHOCH)。这些分子是通过使用耶贝斯40米望远镜对TMC-1进行的深度Q波段谱线调查中的几条发射线检测到的。这些观测结果表明,富含碳链的冷暗云原型TMC-1的氰基多炔峰还包含像HCOOCH和CHOCH这样的含氧化合物的复杂有机分子,这些分子此前在少数冷星际云中被观测到。此外,这是首次在太空中可靠检测到CHOH,也是首次在寒冷环境中检测到CHCHO和CHOH,为冷源中复杂有机分子的谜题增添了新的内容。我们分别得出CHCHO、CHOH、HCOOCH和CHOCH的柱密度为(2.2±0.3)×10厘米、(2.5±0.5)×10厘米、(1.1±0.2)×10厘米和(2.5±0.7)×10厘米。有趣的是,CHOH的丰度与其著名的异构体乙醛(CHCHO)相似,在氰基多炔峰处CHOH/CHCHO约为1。我们讨论了这些分子的潜在形成途径,并认识到需要进一步的实验、理论和天文研究来阐明这些含氧化合物的复杂有机分子在冷星际源中的真正形成机制。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/eaa2/7611417/9a10f9fc1c99/EMS130927-f001.jpg

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