The Circulation of Ionized Gas in the Milky Way Galaxy

Autores/as

  • Andrew Eagon University of Wisconsin-Whitewater

DOI:

https://doi.org/10.17307/wsc.v0i0.140

Palabras clave:

Milky Way, Moment maps, kinematics of Galaxy

Resumen

We use the Wisconsin H-alpha Mapper (WHAM) all sky survey to observe kinematic properties of ionized interstellar gas in the Galaxy. WHAM’s survey is a velocity resolved map of the H-alpha emission from the Milky Way with a one-degree spatial resolution and 12.8 km s-1 velocity resolution. Using this data the first and second moments are calculated and mapped to provide insight on the kinematic properties of the Galaxy. This research was funded by the Wisconsin Space Grant Consortium and supported by the NSF REU site grant to the University of Wisconsin-Madison.

Cover Image of 2015 Proceedings of the Wisconsin Space Conference: Sonex Personal Jet

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Publicado

2016-02-13

Cómo citar

Eagon, A. (2016). The Circulation of Ionized Gas in the Milky Way Galaxy. Proceedings of the Wisconsin Space Conference. https://doi.org/10.17307/wsc.v0i0.140

Número

2015: Innovations in Flight

Sección

Astronomy and Cosmology

Licencia

Creative Commons License
This work is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License.