SIMBAD references

2006A&A...453.1003T - Astronomy and Astrophysics, volume 453, 1003-1026 (2006/7-3)

A SCUBA imaging survey of ultracompact HII regions. The environments of massive star formation.

THOMPSON M.A., HATCHELL J., WALSH A.J., MacDONALD G.H. and MILLAR T.J.

Abstract (from CDS):

We present a SCUBA submillimetre (450 and 850µm) survey of the environment of 105 IRAS point sources, selected from the Wood & Churchwell (1989ApJS...69..831W) and Kurtz et al. (1994ApJS...91..659K) radio ultracompact (UC) HII region surveys. We detected a total of 155 sub-mm clumps associated with the IRAS point sources and identified three distinct types of object: ultracompact cm-wave sources that are not associated with any sub-mm emission (sub-mm quiet objects), sub-mm clumps that are associated with ultracompact cm-wave sources (radio-loud clumps); and sub-mm clumps that are not associated with any known ultracompact cm-wave sources (radio-quiet clumps). 90% of the sample of IRAS point sources were found to be associated with strong sub-mm emission. We consider the sub-mm colours, morphologies and distance-scaled fluxes of the sample of sub-mm clumps and show that the sub-mm quiet objects are unlikely to represent embedded UC HII regions unless they are located at large heliocentric distances. Many of the 2.5' SCUBA fields contain more than one sub-mm clump, with an average number of companions (the companion clump fraction) of 0.90. The clumps are more strongly clustered than other candidate HMPOs and the mean clump surface density exhibits a broken power-law distribution with a break at 3pc. We demonstrate that the sub-mm and cm-wave fluxes of the majority of radio-loud clumps are in excellent agreement with the standard model of ultracompact HII regions. We speculate on the nature of the radio-quiet sub-mm clumps and, whilst we do not yet have sufficient data to conclude that they are in a pre-UC HII region phase, we argue that their characteristics are suggestive of such a stage.

Abstract Copyright:

Journal keyword(s): stars: formation - ISM: HII regions - ISM: dust, extinction - submillimeter - radio continuum: ISM

VizieR on-line data: <Available at CDS (J/A+A/453/1003): table1.dat table2.dat refs.dat

Nomenclature: Table 2, col.(2): [THW2006] GLLL.lll+BB.bbbSMM N=159 = Table 2, col.(1): [THW2006] GLL.ll+BB.bb a N=159.

Simbad objects: 423

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2006A&A...453.1003T and select 'bookmark this link' or equivalent in the popup menu


2019.10.24-02:54:22

© Université de Strasbourg/CNRS

    • Contact