In situ measurement of the cosmic microwave background temperature at a distance of 7.5 kiloparsecs

Astronomy and Astrophysics – Astrophysics

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Formaldehyde, H Ii Regions, Interstellar Gas, Relic Radiation, Very Large Array (Vla), Hydrogen Clouds, Molecular Clouds, Red Shift

Scientific paper

Absorption of orthoformaldehyde (H2CO) toward the giant H II region W51A (G49.5 - 0.4) has been used as a remote probe of the cosmic microwave background (CMB) at a distance of 7.5 kpc. VLA observations of the 6 cm and 2 cm wavelength transitions provided sufficient resolution and sensitivity to resolve condensations within the foregound clouds. Solutions to the equations of statistical equilibrium within each condensation in the context of a large velocity gradient model yielded an estimate for the CMB temperature at 2.1 mm wavelength of 3.2 + or - 0.9 K. The uncertainty is dominated by modeling of collisional pumping by neutral hydrogen molecules (H2).

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