Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988msngr..53...26r&link_type=abstract
ESO Messenger (ISSN 0722-6691), Sept. 1988, p. 26-29.
Astronomy and Astrophysics
Astronomy
2
Galactic Evolution, Radio Galaxies, Star Formation Rate, Cosmology, Radio Astronomy, Red Shift
Scientific paper
It is presently calculated that the best star formation rate yielded by evolutionary models for explaining the emission of the radio galaxy 0902+34 in the K band is an intense burst which began 3 Gyr earlier and persisted for 1 Gyr. An additional present (galaxy frame) burst of 0.1 Gyr explains the V, and partly accounts for the I emission. The dominant stellar component emitting in the K band is on the Asymptotic Giant Branch.
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