On star formation in cooling flows of clusters of galaxies

Details On star formation in cooling flows of clusters of galaxies On star formation in cooling flows of clusters of galaxies

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991an....312..161s&link_type=abstract

Astronomische Nachrichten (ISSN 0004-6337), vol. 312, no. 3, 1991, p. 161-165.

Astronomy and Astrophysics

Astrophysics

1

Cooling Flows (Astrophysics), Galactic Clusters, Star Formation, Stellar Mass, Luminous Intensity, Red Shift

Scientific paper

A correlation between the masses of cooling flows in clusters of galaxies and the absolute magnitudes of the central parts of the brightest galaxies of the clusters is detected. This correlation is consistent with star formation in the cooling flows according to an initial mass function of stars truncated at stellar masses corresponding to absolute magnitudes in the most probable cases between +7 and +2.

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