Brackett-γ Line Survey of the Ionized Hydrogen in the Galactic Plane

Details Brackett-γ Line Survey of the Ionized Hydrogen in the Galactic Plane Brackett-γ Line Survey of the Ionized Hydrogen in the Galactic Plane

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004assl..315...79k&link_type=abstract

How Does the Galaxy Work? A Galactic Tertulia with Don Cox and Ron Reynolds. Edited by Emilio J. Alfaro, Instituto de Astrofisic

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We have carried out a 2.1655 micron Brackett-gamma hydrogen recombination emission line pilot survey of the Galactic plane using a Goddard-Wisconsin cryogenic Fabry-Perot spectrometer. For this survey fields were selected along the Galactic plane from 358° to 43° longitude. The velocity range of the observed emission features ranges from -10 km s-1 to 90 km s-1 (LSR). Typical detected intensities correspond to emission measures of about 1000 cm-6 pc.

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