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2007MNRAS.374..979C - Mon. Not. R. Astron. Soc., 374, 979-998 (2007/January-3)
Absolute diffuse calibration of IRAC through mid-infrared and radio study of HII regions.
COHEN M., GREEN A.J., MEADE M.R., BABLER B., INDEBETOUW R., WHITNEY B.A., WATSON C., WOLFIRE M., WOLFF M.J., MATHIS J.S. and CHURCHWELL E.B.
Abstract (from CDS):
From regression analyses we find that 843-MHz radio fluxes of Hii regions and mid-infrared (MIR) fluxes are linearly related for MSX at 8.3µm and Spitzer at 8.0µm, confirming the earlier MSX result by Cohen & Green. The median ratio of MIR/843-MHz diffuse continuum fluxes is 600x smaller in non-thermal than thermal regions, making it a sharp discriminant. The ratios are largely independent of morphology up to a size of ∼24arcmin. We provide homogeneous radio and MIR morphologies for all sources. MIR morphology is not uniquely related to radio structure. Compact regions may have MIR filaments and/or diffuse haloes, perhaps infrared counterparts to weakly ionized radio haloes found around compact Hii regions. We offer two IRAC colour-colour plots as quantitative diagnostics of diffuse Hii regions.
Abstract Copyright: 2006 The Authors. Journal compilation © 2006 RAS
Journal keyword(s): radiation mechanisms: non-thermal - radiation mechanisms: thermal - ISM: structure - supernova remnants - infrared: ISM - radio continuum: ISM
Nomenclature: Table 1: [CG2001] GLLL.ll+B.bb (No. G311.70+0.31) added.
CDS comments: In Chap. 10 : G313.45-0.13 is a misprint for G311.45-0.13
Simbad objects: 61
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