Please use this identifier to cite or link to this item:
|Title:||GMRT and VLA Observations at 49 cm and 20 cm of the HII Region near l = 24.8d, b = 0.1d|
Roshi, Anish D.
Mohan, Niruj R.
radio recombination lines
|Publisher:||Indian Academy of Sciences, Bangalore, India|
|Citation:||Journal of Astrophysics and Astronomy, 2007, Vol.28, p41-53|
|Abstract:||We report multi-frequency radio continuum and hydrogen radio recombination line observations of HII regions near l = 24.8◦, b = 0.1◦ using the Giant Metrewave Radio Telescope(GMRT) at 1.28 GHz (n = 172), 0.61 GHz (n = 220) and the Very Large Array (VLA) at 1.42 GHz (n = 166). The region consists of a large number of resolved HII regions and a few compact HII regions as seen in our continuum maps, many of which have associated infrared (IR) point sources. The largest HII region at l = 24.83◦ and b = 0.1◦ is a few arcmins in size and has a shell-type morphology. It is a massive HII region enclosing ∼550M with a linear size of 7 pc and an rms electron density of ∼110 cm−3 at a kinematic distance of 6 kpc. The required ionization can be provided by a single star of spectral type O5.5. We also report detection of hydrogen recombination lines from the HII region at l = 24.83◦ and b = 0.1◦ at all observed frequencies near Vlsr = 100 km s−1. We model the observed integrated line flux density as arising in the diffuse HII region and find that the best fitting model has an electron density comparable to that derived from the continuum.We also report detection of hydrogen recombination lines from two other HII regions in the field.|
|Copyright:||Indian Academy of Sciences, Bangalore, India|
|Appears in Collections:||Research Papers (A&A)|
Files in This Item:
|2007 JAA V28 p41-53.pdf|
|Open Access||1.57 MB||Adobe PDF||View/Open Request a copy|
Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.