Star formation in cooling flows in clusters of galaxies

Details Star formation in cooling flows in clusters of galaxies Star formation in cooling flows in clusters of galaxies

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aj.....98.2018m&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 98, Dec. 1989, p. 2018-2043.

Astronomy and Astrophysics

Astrophysics

113

Cooling Flows (Astrophysics), Galactic Clusters, Star Formation, Absorption Spectra, Emission Spectra, Galactic Nuclei, Red Shift, Spectral Line Width, Ultraviolet Spectroscopy

Scientific paper

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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