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Star formation in cooling flows in clusters of galaxies | Synapse

December 1, 1989

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Star formation in cooling flows in clusters of galaxies

JMJ. Regis McNamaraUniversity of Waterloo ROR. W. O’ConnellUniversity of Virginia

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Resumen

Spectrophotometry (wavelength = 3400-5100 A) has been obtained for the nuclei of 13 cD galaxies in cooling flows. Spectral anomalies are found in 8 of the objects, consisting of abnormally strong forbidden O II emission or excess flux effects. Consideration is given to metallicity effects, the relationship between UV excesses and the presence of massive OB stars formed from the cooling flows, and low-level effects related to accretion.

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Cite This Study

McNamara et al. (Fri,) studied this question.

synapsesocial.com/papers/69dabcd80f32475823a3da92 https://doi.org/https://doi.org/10.1086/115275