Physical conditions in Centaurus A’s northern filaments

IF 5.4 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astronomy & Astrophysics Pub Date : 2024-10-21 DOI:10.1051/0004-6361/202450952
Q. Salomé, P. Salomé, B. Godard, P. Guillard, A. Gusdorf
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Abstract

We present the first observations of HCO+(1–0) and HCN(1–0) emission in the northern filaments of Centaurus A with ALMA. HCO+(1–0) is detected in nine clumps of the Horseshoe complex, with similar velocities as the CO(1–0) emission. Conversely, HCN(1–0) is not detected, and we derive upper limits on the flux. At a resolution of ∼40 pc, the line ratio of the velocity-integrated intensities IHCO+/ICO varies between 0.03 and 0.08, while IHCO+/IHCN is higher than unity, with an average lower limit of 1.51. These ratios are significantly higher than what is observed in nearby star-forming galaxies. Moreover, the ratio IHCO+/ICO decreases with increasing CO-integrated intensity, contrary to what is observed in the star-forming galaxies. This indicates that the HCO+ emission is enhanced and may not arise from dense gas within the Horseshoe complex. This hypothesis is strengthened by the average line ratio IHCN/ICO < 0.03, which suggests that the gas density is rather low. Using non-local thermal equilibrium, large velocity gradient modelling with RADEX, we explored two possible phases of the gas, which we call ‘diffuse’ and ‘dense’ and are characterised by a significant difference in the HCO+ abundance relative to CO, respectively NHCO+/NCO = 10−3 and NHCO+/NCO = 3 × 10−5. The average CO(1–0) and HCO+(1–0) integrated intensities and the upper limit on HCN(1–0) are compatible with both diffuse (nH = 103 cm−3, Tkin = 15 − 165 K) and dense gas (nH = 104 cm−3, Tkin > 65 K). The spectral setup of the present observations also covers SiO(2–1). While undetected, the upper limit on SiO(2–1) is not compatible with the RADEX predictions for the dense gas. We conclude that the nine molecular clouds detected in HCO+(1–0) are likely dominated by diffuse molecular gas. While the exact origin of the HCO+(1–0) emission remains to be investigated, it is likely related to the energy injection within the molecular gas that prevents gravitational collapse and star formation.
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半人马座A北侧细丝的物理条件
我们首次利用 ALMA 观测了半人马座 A 北细丝的 HCO+(1-0) 和 HCN(1-0) 发射。在马蹄形复合体的九个团块中探测到了 HCO+(1-0),其速度与 CO(1-0) 辐射相似。相反,HCN(1-0)没有被探测到,我们推导出了通量的上限。在 ∼40 pc 的分辨率下,速度积分强度 IHCO+/ICO 的线比在 0.03 和 0.08 之间变化,而 IHCO+/IHCN 则高于 1,平均下限为 1.51。这些比率明显高于在附近恒星形成星系中观测到的比率。此外,IHCO+/ICO比率随着CO积分强度的增加而降低,这与在恒星形成星系中观测到的情况相反。这表明 HCO+ 的发射是增强的,可能并非来自马蹄形复合星系内的致密气体。相对于 CO 的平均线比 IHCN/ICO + 丰度(分别为 NHCO+/NCO = 10-3 和 NHCO+/NCO = 3 × 10-5)加强了这一假设。CO(1-0)和 HCO+(1-0)的平均综合强度以及 HCN(1-0)的上限与弥漫气体(nH = 103 cm-3,Tkin = 15 - 165 K)和致密气体(nH = 104 cm-3,Tkin > 65 K)相符。本次观测的光谱设置也涵盖了 SiO(2-1)。虽然没有检测到,但 SiO(2-1) 的上限与 RADEX 对致密气体的预测不符。我们的结论是,在 HCO+(1-0)中探测到的九个分子云可能主要是弥漫分子气体。虽然 HCO+(1-0)发射的确切来源还有待研究,但它很可能与分子气体中的能量注入有关,这种能量注入会阻止引力塌缩和恒星形成。
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
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