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2002ApJ...568L..19B - Astrophys. J., 568, L19-L22 (2002/March-3)
Photospheric abundances of the hot stars in NGC 1399 and limits on the Fornax cluster cooling flow.
BROWN T.M., FERGUSON H.C., O'CONNELL R.W. and OHL R.G.
Abstract (from CDS):
Although NGC 1399 is at the center of the Fornax Cluster, we find no evidence for O VI cooling flow emission. The upper limit to λλ1032, 1038 emission is 3.9x10–15 ergs.s–1.cm–2, equivalent to 0.14 M☉ yr–1 and less than the value predicted by simple cooling flow models of the NGC 1399 X-ray luminosity.
Abstract Copyright: ∼
Journal keyword(s): Galaxies: Abundances - Galaxies: Elliptical and Lenticular, cD - Galaxies: Stellar Content - Ultraviolet: Galaxies
Simbad objects: 3
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