arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 2602.10072astro-ph.GA
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SDSS-V局部体积制图器(LVM):螺旋星云公开数据,数据分析流水线数据产品

SDSS-V Local Volume Mapper (LVM): Helix Nebula public data, Data Analysis Pipeline data products

S. F. Sánchez, J. E. Méndez-Delgado, A. Mejía-Narváez, C. Román-Zuñiga, O. V. Egorov, C. Morisset, N. Drory, G. A. Blanc, K. Kreckel, E. J. Johnston, Ivan Yu. K… 展开作者

S. F. Sánchez, J. E. Méndez-Delgado, A. Mejía-Narváez, C. Román-Zuñiga, O. V. Egorov, C. Morisset, N. Drory, G. A. Blanc, K. Kreckel, E. J. Johnston, Ivan Yu. Katkov, A. Roman Lopes, M. A. Villa-Durango, H. Ibarra-Medel, H. -W. Rix, R. de J. Zermeño, J. G. Fernández Trincado, A. Singh, P. García, G. S. Stringfellow, L. Sabin, J. Toalá, R. Orozco Duarte, A. M. Jones

AI总结:

SDSS-V LVM通过高分辨率光谱分析揭示螺旋星云的电离分层结构,展示其在行星状星云研究中的诊断能力。

摘要:

我们利用SDSS-V局部体积制图器(LVM)的数据,对螺旋星云(NGC 7293)进行了空间分辨的光谱分析,采用最近开发的LVM数据分析流水线(LVM-DAP)。覆盖完整的可见光范围(3600-9800 Å)在一个连续的约0.5度场内,LVM数据提供了该典型行星状星云所有主要离子物种的首个六边形采样、宽视场发射线图。所得到的流量、运动学和线比图揭示了该星云已知的电离分层,从紧凑的He++核心到明亮的[O III]环和扩展的低电离包层,使能够与经典孔径光谱学进行详细比较。由于LVM的灵敏度和均匀的空间采样,在星云中检测到许多微弱的极光和诊断线,包括[O III] 4363、[N II] 5755和He I线,允许对弱线形态进行精确测量。推导出的径向趋势证实了 remarkably 低的尘埃含量和主要环内整体电子温度和密度的均匀性。通过Hα追踪的电离气体运动学进一步支持了缓慢扩展、边缘明亮的壳层场景,与先前研究一致。这项工作展示了LVM光谱学对扩展星云的诊断能力,并突显了其恢复复杂电离结构中全局和空间分辨物理条件的能力。

英文摘要:

We present a spatially resolved spectroscopic analysis of the Helix Nebula (NGC 7293) using data from the SDSS-V Local Volume Mapper (LVM), by applying the recently developed LVM Data Analysis Pipeline (LVM-DAP). Covering the full optical range (3600-9800 Å) over a contiguous ~ 0.5 degree field, the LVM data provide the first hexagonally sampled, wide-field emission-line maps of all major ionic species in this archetypal planetary nebula. The resulting flux, kinematic, and line-ratio maps reveal the well-known ionization stratification of the nebula, from the compact He++ core to the bright [O III] ring and the extended low-ionization envelope, enabling a detailed comparison with classical aperture spectroscopy. Owing to the sensitivity and uniform spatial sampling of the LVM, numerous faint auroral and diagnostic lines are detected across the nebula, including [O III] 4363, [N II] 5755, and He I lines, allowing precise measurements of weak-line morphology. The derived radial trends confirm the remarkably low dust content and the overall homogeneity of electron temperature and density across the main ring. Ionized-gas kinematics traced by Hα further support the scenario of a slowly expanding, limb-brightened shell consistent with previous studies. This work demonstrates the diagnostic power of LVM spectroscopy for extended nebulae and highlights its capability to recover both global and spatially resolved physical conditions across complex ionized structures.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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