4 毫米波长范围内恒星形成区 DR21OH 的光谱巡天

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Astronomy Reports Pub Date : 2024-02-25 DOI:10.1134/S106377292312003X
S. V. Kalenskii, E. A. Mikheeva
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摘要

摘要 介绍了在 4 毫米波长范围内对大质量恒星形成区 DR21OH 进行光谱调查的结果。共探测到 69 种分子及其同素异形体,既有简单的二原子或三原子物质,如 SO、SiO 和 CCH,也有复杂的有机分子,如 CH3OCHO 或 CH3OCH3。所获得的结果定性地重复了在 3 毫米处对同一来源进行勘测的结果。在 3 毫米和 4 毫米处发现的分子清单在很大程度上是重叠的。不过,在 4 毫米波长处,我们发现了一些在 3 毫米波长范围内不允许发生跃迁的物质,如 DCN、DNC 或 SO+。在 4 毫米波长处探测到的大部分分子都是密核常见的分子,如 HC3N 或 CH3CCH,但探测到的一些物种是热核的典型分子。后者包括复杂的有机分子 CH3OCHO、CH3CH2OH、CH3OCH3 等。不过,探测到的这些分子的辐射可能只是在加热到 30 K 的气体中产生的。通过谱线叠加发现了九种分子,包括复杂物种 CH3C3N、CH3CH2CN、CH3COCH3。这证明了该方法在分子云研究中的应用前景。
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Spectral Survey of the Star Formation Region DR21OH in the 4-mm Wavelength Range

The results of a spectral survey of the region of massive star formation DR21OH in the 4-mm wavelength range are presented. Sixty-nine molecules and their isotopologues have been detected, ranging from simple diatomic or triatomic species such as SO, SiO and CCH, to complex organic molecules such as CH3OCHO or CH3OCH3. The obtained results qualitatively repeat the results of the survey of the same source at 3 mm. The inventories of molecules found at 3 and 4 mm overlap to a great extent. However, at 4 mm we found a number of species that have no allowed transitions in the 3-mm wavelength range, e.g., DCN, DNC, or SO+. The bulk of the molecules detected at 4 mm are those that are common for dense cores, e.g., HC3N or CH3CCH, but some of the detected species are typical for hot cores. The latter include complex organic molecules CH3OCHO, CH3CH2OH, CH3OCH3, etc. However, the detected emission of these molecules probably arises in a gas heated to 30 K only. Nine molecules, including complex species CH3C3N, CH3CH2CN, CH3COCH3, were found by spectral line stacking. This demonstrates the prospects of the method in the study of molecular clouds.

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来源期刊
Astronomy Reports
Astronomy Reports 地学天文-天文与天体物理
CiteScore
1.40
自引率
20.00%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Astronomy Reports is an international peer reviewed journal that publishes original papers on astronomical topics, including theoretical and observational astrophysics, physics of the Sun, planetary astrophysics, radio astronomy, stellar astronomy, celestial mechanics, and astronomy methods and instrumentation.
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