New CO observations of the high-latitude molecular cloud MBM 55, near IRAS 230604 + 145055

Astronomy and Astrophysics – Astronomy

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Carbon Monoxide, Infrared Astronomy Satellite, Interstellar Gas, Millimeter Waves, Molecular Clouds, Star Formation, Astronomical Maps, Line Spectra, Rotational Spectra

Scientific paper

Two spatially and kinematically distinct clumps of molecular gas were discovered in the vicinity of the point source IRAS 2306 + 1451 in the MBM 55. The two clumps are red and blue-shifted with respect to the narrow (C-13)O line core velocity, and are located on opposite sides of the IRAS source. The separation of 3 arcmin between the peaks of the red and blue emission corresponds to less than 0.16 pc, uncorrected for an unknown projection effect.

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