AI 中文总结
研究活动星系核中风与喷流关系，通过检验多种星系排除简单尺度不变性，发现黑洞质量和自旋不能解释二分法，指出盘与黑洞角动量方向是关键参数，至少两种风 - 喷流状态运作，确定了AGN子类中行为细节。
AI 中文摘要
X射线双星中盘风与相对论喷流之间已确立的反相关关系，常被在尺度不变的黑洞吸积背景下解释。若如此，活动星系核（AGN）应呈现直接的质量缩放类似物。我们在FRII射电类星体、射电宁静类星体以及螺旋星系中带喷流和不带喷流的窄线塞弗特1星系（NLS1）等中检验了这一预测。结果排除了简单的尺度不变性。最高速度的风仅出现在射电宁静类星体中，而强大的FRII类星体尽管黑洞质量相同，但风系统地较弱。带喷流的NLS1显示出与X射线双星行为一致的强风抑制，而FRII类星体处于喷流和风共存的独特状态。仅黑洞质量和自旋大小无法解释这种二分法。我们认为盘相对于黑洞的角动量方向（对齐与反对齐或共旋转与反旋转）是关键参数：长期供能的螺旋系统和大多数合并后系统倾向于共旋转，这与紧凑的内最稳定圆轨道半径、高辐射效率、强风以及喷流抑制相关，而受合并影响的椭圆星系中的反旋转子集可以维持强大的喷流以及适度的风。此外，虽然螺旋AGN和合并驱动的射电宁静类星体经历类似的强喷流/风反相关，但它们不能被视为X射线双星的严格缩放类似物，因为X射线双星会经历涉及AGN中不存在的磁通量重新分布的快速状态转变。因此，至少有两种不同的风 - 喷流状态在质量尺度上运作。我们确定了AGN子类中这种行为的细节。
英文摘要
The well-established anti-correlation between disk winds and relativistic jets in X-ray binaries is often interpreted in a scale-invariant black hole accretion context. If so, active galactic nuclei (AGN) should exhibit a direct mass-scaled analog. We test this prediction across FRII radio quasars, radio-quiet quasars, and jetted and non-jetted Narrow Line Seyfert 1 galaxies (NLS1) in spirals, among others. They exclude simple scale invariance. The highest-velocity winds occur exclusively in radio-quiet quasars, while powerful FRII quasars host systematically weaker winds despite equally large black hole masses. Jetted NLS1s show strong wind suppression consistent with X-ray binary behavior, whereas FRII quasars occupy a distinct regime in which jets and winds coexist. Black hole mass and spin magnitude alone cannot account for this dichotomy. We argue that the angular momentum direction of the disk relative to that of the black hole (aligned versus anti-aligned or co-rotation versus counter-rotation) is the critical parameter: secularly fueled spiral systems and most post-merger systems favor co-rotation, which is associated with compact ISCO radii, high radiative efficiency, strong winds, and jet suppression, while the counter-rotating subset of merger-influenced ellipticals can sustain powerful jets alongside moderate winds. Moreover, while spiral AGN and merger-driven radio-quiet quasars experience similar strong jet/wind anti-correlation, they cannot be treated as strict scaled analogs of X-ray binaries, which undergo rapid state transitions involving magnetic flux redistribution absent in AGN. At least two distinct wind-jet regimes therefore operate across the mass scale. We identify the details of this behavior across AGN subclasses.
Comments17 pages, 3 figures, 2 tables, Accepted for publication in the Galaxies journal
Journal refGalaxies 2026, 14(4), 72
