首页> 外文期刊>The Astrophysical Journal. Letters >FILAMENTARY LARGE-SCALE STRUCTURE TRACED BY SIX Lyα BLOBS AT z = 2.3
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FILAMENTARY LARGE-SCALE STRUCTURE TRACED BY SIX Lyα BLOBS AT z = 2.3

机译:六个Lyα斑点在z = 2.3时跟踪的丝状大尺度结构

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摘要

Extended nebulae of Lyα emission (“Lyα blobs”) are known to be associated with overdense regions at high redshift. Here we present six large Lyα blobs in a previously known protocluster with galaxy overdensity δ ~ 7 at z = 2.3; this is the richest field of giant Lyα blobs detected to date. The blobs have linear sizes of ≥100 kpc and Lyα luminosities of ~10~(43) erg s~(-1). The positions of the blobs define two linear filaments with an extent of at least 12 comoving Mpc; these filaments intersect at the center of one of the blobs. Measurement of the position angles of the blobs indicates that five of the six are aligned with these filaments to within ~10°, suggesting a connection between the physical processes powering extended Lyα emission and those driving structure on larger scales.
机译:众所周知,Lyα发射的扩展星云(“Lyα斑点”)与高红移区的过密区域有关。在这里,我们在一个先前已知的原团中展示了六个大的Lyα斑点,在z = 2.3时星系的密度为δ〜7。这是迄今为止检测到的最大的Lyα斑点最丰富的区域。斑点的线性大小为≥100kpc,Lyα光度为〜10〜(43)erg s〜(-1)。斑点的位置定义了两个线性细丝,其长度至少为12个共同移动的Mpc。这些细丝在斑点之一的中心相交。斑点位置角的测量结果表明,六个斑点中的五个与这些细丝在约10°内对齐,这表明为扩展的Lyα发射提供动力的物理过程与更大尺度上的驱动结构之间存在联系。

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