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2.3 GHz Radio Emission From Sco OB2

Published online by Cambridge University Press:  14 August 2015

E.E. Baart ,
G. de Jager  and
P. I. Mountfort
E.E. Baart
Affiliation:
Rhodes University, Grahamstown, South Africa
G. de Jager
Affiliation:
Rhodes University, Grahamstown, South Africa
P. I. Mountfort
Affiliation:
Rhodes University, Grahamstown, South Africa

Extract

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The Sco OB2 Association is convenient for investigation as it has a high galactic latitude and is therefore remote from the confusion of the galactic plane. Its distance is accurately known and this permits fairly precise estimates to be made of the Lyman continuum photon fluxes responsible for the radio emission. It includes the ρ Ophiuci dark cloud where star formation is occurring.

Type
August 27 Introduction, Associations, Galactic Structure
Information
Symposium - International Astronomical Union , Volume 85: Star Clusters , 1980 , pp. 105 - 106
Copyright
Copyright © Reidel 1980