A narrow linear object extending ~60kpc from the centre of a galaxy at redshift z ~ 1 has been recently discovered and interpreted as a shocked gas filament forming stars. The host galaxy presents an irregular morphology, implying recent merger event...
We present a theoretical framework for linking quasar properties, such as quasar age, to the surrounding Ly α emission intensity. In particular, we focus on a method for mapping the large-scale structure of Ly α emission intensity with galaxy spectra...
A narrow linear object extending ~60kpc from the centre of a galaxy at redshift z ~ 1 has been recently discovered and interpreted as a shocked gas filament forming stars. The host galaxy presents an irregular morphology, implying recent merger event...
令和5年 8月 13 : 30 巨大ブラックホール , 流体力学 , CGM
We present a theoretical framework for linking quasar properties, such as quasar age, to the surrounding Ly α emission intensity. In particular, we focus on a method for mapping the large-scale structure of Ly α emission intensity with galaxy spectra...
令和5年 7月 13 : 30 ライマン・アルファ輝線天体 , クエーサー , 巨大ブラックホール
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