( Artist’s illustration of CRISTAL-13. Dust-rich regions obscure newborn stars, whose energy is re-emitted at ALMA’s millimeter wavelengths. Right: young star clusters clear the dust and shine visibly in JWST and HST images. Credit: NSF/AUI/NRAO/B. Saxton ) ( A family portrait of galaxies from the CRISTAL survey. Red shows cold gas traced by ALMA's [CII] observations. Blue and green represent starlight captured by the Hubble and James Webb Space Telescopes. Credit: ALMA (ESO/NAOJ/NRAO) / HST / JWST / R. Herrera-Camus ) ( Zoom into the emission from an early galaxy observed in the CRISTAL survey. From left to right, the image shows stellar light captured by the James Webb and Hubble space telescopes, as well as the cold gas and rotation of the galaxy traced by ALMA through ionized carbon emission. Credit: ALMA / HST / JWST / R. Herrera-Camus ) 세계에서 가장 강력한 전파 망원경 중 하나인 ALMA (Atacama Large Millimeter/submillimeter Array)가 우주 초기 생성 단계에 있는 은하 구성 물질의 구조를 밝혀냈습니다. 크리스탈 서베이 (CRISTA...
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