SIMBAD references

2002ApJ...568..754K - Astrophys. J., 568, 754-760 (2002/April-1)

An ionized accretion flow in the ultracompact H II region G10.6-0.4.

KETO E.

Abstract (from CDS):

Analysis of the H66α radio recombination line velocities in the ultracompact H II region G10.6-0.4 indicates inward motion of the ionized gas within the H II region. Comparison with the velocities of molecular lines from the surrounding neutral gas suggests that a molecular accretion flow passes through the ionization boundary of the H II region and continues inward as an ionized accretion flow. Interpreted in the context of a model for star formation in hot molecular cores, these observations indicate that G10.6-0.4 is at a stage of development just after the massive star or stars at the center of the accretion flow have first formed an ionized H II region within the hot molecular core.

Abstract Copyright:

Journal keyword(s): Accretion, Accretion Disks - ISM: H II Regions - Stars: Individual: Alphanumeric: G10.6-0.4

CDS comments: G 9.62+0.31 is a misprint for G 9.62+0.19 and G 29.96+0.02 for G 29.96-0.02.

Simbad objects: 15

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2019.12.15-12:23:51

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