The discovery of clumpy structure in the diffuse gas towards Cyg OB2 No. 12

Details The discovery of clumpy structure in the diffuse gas towards Cyg OB2 No. 12 The discovery of clumpy structure in the diffuse gas towards Cyg OB2 No. 12

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mnras.337..495s&link_type=abstract

Monthly Notice of the Royal Astronomical Society, Volume 337, Issue 2, pp. 495-498.

Astronomy and Astrophysics

Astronomy

9

Stars: Individual: Cyg Ob2 No. 12, Ism: Clouds, Ism: Molecules

Scientific paper

We have mapped the 13CO (1-0) line in a region of sky towards the star Cyg OB2 No. 12. The observations rule out the possibility that the molecular material along the line of sight is distributed over a long path of very dilute gas. Instead, we present unambiguous evidence of well-defined kinematical structures, which might be assembled to form a cloud complex. The chemistry that leads to H+3 appears decoupled from that responsible for the production of heavier species.

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