Cooling flows and a giant red envelope galaxy

Details Cooling flows and a giant red envelope galaxy Cooling flows and a giant red envelope galaxy

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.237p..27j&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 237, March 1, 1989, p. 27P-30P. Research supported by t

Astronomy and Astrophysics

Astrophysics

13

Cooling Flows (Astrophysics), Galactic Clusters, Red Shift, Stellar Mass, X Ray Sources, Galactic Nuclei, Heao 2, Mass Distribution

Scientific paper

It is shown that recent i-band observations of a giant red envelope
galaxy (GREG) are consistent with a population of low-mass stars which
has been forming from a cooling flow. This is the first time that the
bulk of the accretion population in a cooling flow has been identified.

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