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IFU investigation of possible Lyman continuum escape from Mrk 71/NGC 2366 ?

机译:IFU对Mrk 71 / NGC 2366中可能发生的莱曼连续体逃逸的调查

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Context . Mrk 71/NGC 2366 is the closest green pea (GP) analog and candidate Lyman Continuum (LyC) emitter. Recently, 11 LyC-leaking GPs have been detected through direct observations of the ionizing continuum, making this the most abundant class of confirmed LyC-emitters at any redshift. High resolution, multiwavelength studies of GPs can lead to an understanding of the method(s), through which LyC escapes from these galaxies. Aims . The proximity of Mrk 71/NCG 2366 offers unprecedented detail on the inner workings of a GP analog, and enables us to identify the mechanisms of LyC escape. Methods . We used 5825–7650 ? integral field unit PMAS observations to study the kinematics and physical conditions in Mrk 71. An electron density map was obtained from the [S? II ] ratio. A fortuitous second order contamination by the [O? II ] λ 3727 doublet enabled the construction of an electron temperature map. Resolved maps of sound speed, thermal broadening, “true” velocity dispersion, and Mach number were obtained and compared to the high resolution magnetohydrodynamic SImulating the LifeCycle of molecular Clouds (SILCC) simulations. Results . Two regions of increased velocity dispersion indicative of outflows are detected to the north and south of the super star cluster, knot B, with redshifted and blueshifted velocities, respectively. We confirm the presence of a faint broad kinematical component, which is seemingly decoupled from the outflow regions, and is fainter and narrower than previously reported in the literature. Within uncertainties, the low- and high-ionization gasses move together. Outside of the core of Mrk 71, an increase in Mach numbers is detected, implying a decrease in gas density. Simulations suggest this drop in density can be as high as ~4 dex, down to almost optically thin levels, which would imply a nonzero LyC escape fraction along the outflows even when assuming all of the detected H? I gas is located in front of Mrk 71 in the line of sight. Conclusions . Our results strongly indicate that kinematical feedback is an important ingredient for LyC leakage in GPs.
机译:语境。 Mrk 71 / NGC 2366是最接近的绿豌豆(GP)类似物和候选Lyman Continuum(LyC)发光体。最近,通过直接观察电离连续体已检测到11个LyC泄漏GP,这使其在任何红移条件下都是最丰富的已确认LyC发射极。 GP的高分辨率,多波长研究可以导致人们理解LyC从这些星系中逃脱的方法。目的。 Mrk 71 / NCG 2366的邻近性为GP模拟的内部运作提供了前所未有的细节,使我们能够识别LyC逃逸的机制。方法 。我们使用5825-7650吗?积分场单元PMAS观测,以研究Mrk 71的运动学和物理条件。电子密度图从[S? II]比率。 [O?是偶然的二阶污染。 II]λ3727 doublet能够构建电子温度图。获得了声速,热展宽,“真实”速度色散和马赫数的解析图,并将其与高分辨率磁流体动力学模拟分子云生命周期(SILCC)模拟进行了比较。结果。在超级恒星团的北部和南部,分别以红移和蓝移的速度检测到两个指示外流的速度散布增加的区域。我们证实存在弱的广泛运动学成分,该成分似乎与流出区域分离,并且比文献中先前报道的更模糊,更窄。在不确定性范围内,低电离气体和高电离气体会一起移动。在Mrk 71的核心外部,检测到马赫数增加,这意味着气体密度降低。模拟表明,这种密度下降可能高达〜4 dex,下降到几乎光学上的薄水平,这意味着即使假设所有检测到的H 2+,沿着流出的LyC逸出率也不为零。我气位于视线内的Mrk 71前面。结论。我们的结果强烈表明,运动学反馈是GP中LyC泄漏的重要因素。

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