Ultracompact HiiRegions with Extended Radio‐Continuum Emission
Open Access
- 20 March 1999
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 514 (1) , 232-248
- https://doi.org/10.1086/306928
Abstract
We have conducted a 3.6 cm radio-continuum survey with the VLA in its compact D-array to look for extended radio-continuum emission around known ultracompact H II regions. We find extended emission in 12 out of 15 fields. The extended emission ranges in size up to 5', with typical diameters of 60'', or 2 pc. In some cases, the extended component produces an order of magnitude more flux than the ultracompact component. It is possible that the extended emission is from H II regions not connected with the ultracompact H II regions, but on the basis of the morphology of the emission, we believe that it is possible or even likely that the ultracompact and extended emission are directly connected in about half of the sources. The possible consequences of directly connected extended emission are profound. We may be forced to reconsider the definition of an ultracompact H II region and consider models in which dense, ultracompact ionized components are embedded in less dense, more extended regions.Keywords
This publication has 43 references indexed in Scilit:
- The NRAO VLA Sky SurveyThe Astronomical Journal, 1998
- On the Relative Importance of Photoevaporative and Hydrodynamic Effects in the Ablation of Self‐gravitating Globules in Compact HiiRegionsThe Astrophysical Journal, 1997
- Galactic Temperature and Metallicity Gradients from Ultracompact H II RegionsThe Astrophysical Journal Supplement Series, 1996
- Clumpy ultracompact H II regions – I. Fully supersonic wind-blown modelsMonthly Notices of the Royal Astronomical Society, 1995
- A 5 GHz VLA survey of the galactic planeThe Astrophysical Journal Supplement Series, 1994
- A close-up view of the S87 molecular outflowThe Astrophysical Journal, 1989
- VLA observations of H2CO in absorption against the cosmic background radiation - Clumps in the S140 molecular cloudThe Astrophysical Journal, 1987
- Radio images of the bipolar H II region S106The Astrophysical Journal, 1983
- Ionized gas in active molecular cloud coresThe Astrophysical Journal, 1983
- New multiple systems in molecular cloudsThe Astrophysical Journal, 1979