Interstellar formaldehyde in Sagittarius B2

Astronomy and Astrophysics – Astronomy

Scientific paper

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Absorption Spectra, Formaldehyde, Interstellar Matter, Molecular Absorption, Optical Thickness, Radial Velocity, Radiative Recombination, Radio Astronomy

Scientific paper

Measurements of the 6.2-cm absorption line of the formaldehyde (H2CO) molecule have been obtained with a radio telescope having a resolution of 0.8 x 12 arcmin. The distribution of H2CO optical depth over the radio source Sgr B2 indicates that a gas envelope 11 pc in diameter may be present with a mean radial velocity close to the recombination-line velocities. The envelope is contracting at a rate of 20-25 km/sec and rotating at a peripheral velocity of 15 km/sec. The contraction in the central part of the molecular cloud surrounding Sgr B2 implies that it has a very short lifetime: roughly 5 x 10 to the 5th yr for matter in free fall.

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