Molecular Gas Near Unusual Galactic Center Radio Source N3

Ludovici, Dominic A.

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https://hdl.handle.net/2142/51210 Copy

Description

Title

Molecular Gas Near Unusual Galactic Center Radio Source N3

Author(s)

Ludovici, Dominic A.

Contributor(s)

• Lang, Cornelia
• Toomey, James

Issue Date

2014-06-16

Keyword(s)

Astronomy

Abstract

Near the Galactic center, the presence of the supermassive black hole, high dust temperatures, and large densities produce an unique environment within our galaxy. Unfortunately, optical light in this region is obscured by dust, making optical observations difficult or impossible. By utilizing radio telescopes, we can peer through the dust to examine the inner workings of this fascinating region. Using the Very Large Array, we examined the Galactic center radio source N3, a point source located within the Radio Arc. Our observations examined both molecular line and continuum emission from the region at frequencies from 2 GHz to 49 GHz. Several molecular species are detected around N3. Using molecular line analysis, N3's spectral index, physical size limits, and possible interactions between N3 and the Radio Arc, we examine the physical nature of N3 and outline further work needed to complete the analysis of this interesting source.

Publisher

International Symposium on Molecular Spectroscopy

Type of Resource

text

Language

English

Permalink

http://hdl.handle.net/2142/51210

DOI

https://doi.org/10.15278/isms.2014.MF06

Copyright and License Information

Copyright 2014 by the authors. Licensed under a Creative Commons Attribution 4.0 International License. http://creativecommons.org/licenses/by/4.0/

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