Observations of the intercloud HI-gas in the directions of Cassiopeia A and Cygnus A

Astronomy and Astrophysics – Astronomy

Scientific paper

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Cassiopeia A, Hydrogen Ions, Interstellar Gas, Radio Sources (Astronomy), Absorption Spectra, Gas Temperature, H Lines, Microwave Emission, Optical Thickness, Radio Telescopes, Spin Temperature, Stellar Temperature

Scientific paper

Observations of the 21-cm line absorption against the two strongest radio sources, Cas A and Syg A, made with the 100-m telescope of the Effelsberg Observatory at 1420 MHz are discussed. The continuum temperatures obtained with the Effelsberg telescope are 3000 K and 2200 K for Cas A and Cyg A, respectively. Graphs showing the 21-cm line spectra in the direction of Cas A and in the direction of Cyg A are presented, along with graphs showing the spin temperature and optical depth in these two directions.

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