Imaging galactic diffuse clouds: CO emission, reddening and turbulent flow in the gas around ζ Ophiuchi

Context. Most diffuse clouds are only known as kinematic features in absorption spectra, but those with appreciable H2 content may be visible in the emission of such small molecules as CH, OH, and CO. Aims. We interpret in greater detail the extensive observations of 12CO emission from diffuse gas s...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2009-05, Vol.499 (2), p.503-513
Hauptverfasser:	Liszt, H. S., Pety, J., Tachihara, K.
Format:	Artikel
Sprache:	eng
Schlagworte:	astrochemistry Astronomy Astrophysics Earth, ocean, space Exact sciences and technology Galactic Astrophysics ISM: clouds ISM: molecules Physics Sciences of the Universe
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