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Clues for stellar formation in NGC 1275 cooling flow

Published online by Cambridge University Press:  12 April 2016

Pierre Ferruit  and
Emmanuel Pécontal
Pierre Ferruit
Affiliation:
Observatoire de Lyon, 69561 St-Genis-Laval CEDEX, France
Emmanuel Pécontal
Affiliation:
Observatoire de Lyon, 69561 St-Genis-Laval CEDEX, France

Abstract

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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

Type
3. Integral Field Spectrographs and Spectrometers
Information
International Astronomical Union Colloquium , Volume 149: Tridimensional Optical Spectroscopic Methods in Astrophysics , 1995 , pp. 257 - 260
Copyright
Copyright © Astronomical Society of the Pacific 1995

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