The Cygnus X region. XVI - The ionized gas behind the dark cloud between the North America and Pelican nebulae

Details The Cygnus X region. XVI - The ionized gas behind the dark cloud between the North America and Pelican nebulae The Cygnus X region. XVI - The ionized gas behind the dark cloud between the North America and Pelican nebulae

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...148..439h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 148, no. 2, July 1985, p. 439-442.

Astronomy and Astrophysics

Astronomy

6

H Alpha Line, Interstellar Gas, Ionized Gases, Nebulae, Radial Velocity, Radio Spectra, H Ii Regions, Radio Astronomy

Scientific paper

Radio recombination line observations are presented for the ionized gas at selected positions behind the dark cloud separating the North America and Pelican nebulae. The high angular resolution of about 3 arcmin makes it possible to sample the different structural components. The lines are dominated by ionized gas physically similar to that of the visible nebulae. A further extended background source is identified and briefly discussed in terms of an Ori A-type H II region in the Perseus spiral arm.

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