Deep H-alpha survey of gaseous emission regions in the Milky Way and the Magellanic Clouds

Details Deep H-alpha survey of gaseous emission regions in the Milky Way and the Magellanic Clouds Deep H-alpha survey of gaseous emission regions in the Milky Way and the Magellanic Clouds

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991msngr..64...44a&link_type=abstract

ESO Messenger (ISSN 0722-6691), no. 64, p. 44-50.

Computer Science

Performance

37

Carbon Monoxide, Emission Spectra, H Alpha Line, Magellanic Clouds, Milky Way Galaxy, Fabry-Perot Interferometers, Molecular Clouds

Scientific paper

A deep H-alpha survey was conducted to obtain radial velocities of the ionized gas and the structure of the southern H II regions in the Galaxy and in the Magellanic Clouds. The telescope and high-performance software are described, and the reasons for the use of a 36 cm telescope and a photon-counting camera are presented. Some early survey results are reported.

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