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The Early Evolution of Massive Stars: Radio Recombination Line Spectra

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© 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Eric Keto et al 2008 ApJ 672 423 DOI 10.1086/522570

0004-637X/672/1/423

Abstract

Velocity shifts and differential broadening of radio recombination lines are used to estimate the densities and velocities of the ionized gas in several hypercompact and ultracompact H II regions. These small H II regions are thought to be at their earliest evolutionary phase and associated with the youngest massive stars. The observations suggest that these H II regions are characterized by high densities, supersonic flows, and steep density gradients, consistent with accretion and outflows that would be associated with the formation of massive stars.

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10.1086/522570