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Clues for stellar formation in NGC 1275 cooling flow
Published online by Cambridge University Press: 12 April 2016
Abstract
3D spectrography of the inner regions of NGC 1275 has been performed using the integral field spectrograph TIGER. It revealed an association between star clusters and some line emitting gas components, likely to be filaments material. This may indicates that the clusters originate from star formation in the cooling flow
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- 3. Integral Field Spectrographs and Spectrometers
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- Copyright © Astronomical Society of the Pacific 1995