Imaging galactic diffuse gas: Bright, turbulent CO surrounding the line of sight to NRAO150

Abstract

To understand the environment and extended structure of the host galactic gas whose molecular absorption line chemistry, we previously observed along the microscopic line of sight to the blazar/radiocontinuum source NRAO150 (aka B0355+508), we used the IRAM 30m Telescope and Plateau de Bure Interferometer to make two series of images of the host gas: i) 22.5 arcsec resolution single-dish maps of 12CO J=1-0 and 2-1 emission over a 220 arcsec by 220 arcsec field; ii) a hybrid (interferometer+singledish) aperture synthesis mosaic of 12CO J=1-0 emission at 5.8 arcsec resolution over a 90 arcsec-diameter region. CO components that are observed in absorption at a moderate optical depth (0.5) and are undetected in emission at 1 arcmin resolution toward NRAO 150 remain undetected at 6 arcsec resolution. This implies that they are not a previously-hidden large-scale molecular component revealed in absorption, but they do highlight the robustness of the chemistry into regions where the density and column density are too low to produce much rotational excitation, even in CO. Bright CO lines around NRAO150 most probably reflect the variation of a chemical process, i.e. the C+-CO conversion. However, the ultimate cause of the variations of this chemical process in such a limited field of view remains uncertain.

arXiv comment18 pages, 22 PostScript files giving 14 figures. Accepted for publication in Astronomy & Astrophysics in the letter section. Uses aa LaTeX macros

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• The first steps of Interstellar Phosphorus Chemistry
• How well does CO emission measure the H${}_2$ mass of MCs?
• Quantum Calculation of Inelastic CO Collisions with H: I. rotational quenching of low-lying rotational levels
• Imaging galactic diffuse clouds: CO emission, reddening and turbulent flow in the gas around Zeta Oph
• H2CO and CS in diffuse clouds: Excitation and abundance
• Probing the cold and warm molecular gas in the Whirlpool Galaxy: Herschel SPIRE-FTS Observations of the central region of M51 (NGC 5194)
• Study of Interstellar Molecular Clouds using Formaldehyde Absorption toward Extragalactic Radio Sources
• The CO-H2 conversion factor of diffuse ISM: Bright 12CO emission also traces diffuse gas