SIMBAD references

2006MNRAS.368.1843F - Mon. Not. R. Astron. Soc., 368, 1843-1855 (2006/June-1)

Radio and infrared recombination studies of the southern massive star forming region G333.6-0.2.

FUJIYOSHI T., SMITH C.H., CASWELL J.L., MOORE T.J.T., LUMSDEN S.L., AITKEN D.K. and ROCHE P.F.

Abstract (from CDS):

We present high spatial resolution radio and near-infrared hydrogen recombination line observations of the southern massive star forming region G333.6-0.2. The 3.4-cm continuum peak is found slightly offset from the infrared (IR) source. The H90α spectra show for the first time a double-peak profile at some positions. The complex velocity structure may be accounted for by champagne outflows, which may also explain the offset between the radio and IR sources. The 2.17-µm Brγ image and H90α map are combined to construct an extinction map which shows a trend probably set by the blister nature of the Hii region. The total number of Lyman continuum photons in the central 50-arcsec is estimated to be equivalent to that emitted by up to 19 O7V stars.

Abstract Copyright: 2006 The Authors. Journal compilation © 2006 RAS

Journal keyword(s): Hii regions - ISM: individual: G333.6-0.2 - infrared: ISM - radio continuum: ISM - radio lines: ISM

Simbad objects: 5

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2006MNRAS.368.1843F and select 'bookmark this link' or equivalent in the popup menu


2021.07.25-21:00:54

© Université de Strasbourg/CNRS

    • Contact