Abstract
X-ray observations have led to the conclusion that many galaxy clusters are hosting cooling flows. The brightest cluster galaxies could have accreted masses of the order of 1011-1012 M ⊙, but is still uncertain what the final fate of the accreted gas may be.
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© 1996 Springer Science+Business Media Dordrecht
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Cardiel, N., Gorgas, J., Aragon-Salamanca, A. (1996). Spectroscopic Evidences for Star Formation in Cooling Flow Galaxies. In: Bender, R., Davies, R.L. (eds) New Light on Galaxy Evolution. International Astronomical Union / Union Astronomique Internationale, vol 171. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0229-9_61
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DOI: https://doi.org/10.1007/978-94-009-0229-9_61
Publisher Name: Springer, Dordrecht
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