Detection of the 205 μm [N II] line from the Carina Nebula

We report the first detection of the 205 μm 3P1img1.gif P0 [N II] line from a ground-based observatory using a direct detection spectrometer. The line was detected from the Carina star formation region using the South Pole Imaging Fabry-Perot Interferometer (SPIFI) on the Antarctic Submillimeter Tel...

Full description

Bibliographic Details
Published in:The Astrophysical Journal
Main Authors: Oberst, T. E., Parshley, S. C., Stacey, G. J., Nikola, T., Löhr, A., Harnett, J. I., Tothill, N. F. H., Lane, A. P., Stark, A. A., Tucker, Carole
Format: Article in Journal/Newspaper
Language:unknown
Published: IOP Publishing 2006
Subjects:
QB Astronomy
Antarctic
South Pole
The Antarctic
Antarc*
South pole
Online Access:https://orca.cardiff.ac.uk/id/eprint/46320/
https://doi.org/10.1086/510289
Description
Summary:We report the first detection of the 205 μm 3P1img1.gif P0 [N II] line from a ground-based observatory using a direct detection spectrometer. The line was detected from the Carina star formation region using the South Pole Imaging Fabry-Perot Interferometer (SPIFI) on the Antarctic Submillimeter Telescope and Remote Observatory (AST/RO) at the South Pole. The [N II] 205 μm line strength indicates a low-density (n ~ 32 cm-3) ionized medium, similar to the low-density ionized halo previously reported in its [O III] 52 and 88 μm line emission. When compared with the Infrared Space Observatory [C II] observations of this region, we find that 27% of the [C II] line emission arises from this low-density ionized gas, but the large majority (~73%) of the observed [C II] line emission arises from the neutral interstellar medium. This result supports and underpins prior conclusions that most of the observed [C II] 158 μm line emission from Galactic and extragalactic sources arises from the warm, dense photodissociated surfaces of molecular clouds. The detection of the [N II] line demonstrates the utility of Antarctic sites for THz spectroscopy.

Similar Items