The JCMT 12CO(3–2) survey of the Cygnus X region I. A pathfinder

  1. Get@NRC: The JCMT 12CO(3–2) survey of the Cygnus X region I. A pathfinder (Opens in a new window)
DOIResolve DOI:
AuthorSearch for: ; Search for: ; Search for: ; Search for: ; Search for:
Journal titleAstronomy & Astrophysics
Article numberA79
AbstractContext. Cygnus X is one of the most complex areas in the sky, rich in massive stars; Cyg OB2 (2600 stars, 120 O stars) and other OB associations lie within its boundaries. This complicates interpretation, but also creates the opportunity to investigate accretion into molecular clouds and many subsequent stages of star formation, all within one small field of view. Understanding large complexes like Cygnus X is the key to understanding the dominant role that massive star complexes play in galaxies across the Universe. Aims. The main goal of this study is to establish feasibility of a high-resolution CO survey of the entire Cygnus X region by observing part of it as a pathfinder, and to evaluate the survey as a tool for investigating the star-formation process. We can investigate the mass accretion history of outflows, study interaction between star-forming regions and their cold environment, and examine triggered star formation around massive stars. Methods. A 2° × 4° area of the Cygnus X region has been mapped in the 12CO(3–2) line at an angular resolution of 15′′ and a velocity resolution of ~0.4 km s-¹ using HARP-B and ACSIS on the James Clerk Maxwell Telescope. The star formation process is heavily connected to the life-cycle of the molecular material in the interstellar medium. The high critical density of the 12CO(3–2) transition reveals clouds in key stages of molecule formation, and shows processes that turn a molecular cloud into a star. Results. We observed ~15% of Cygnus X, and demonstrated that a full survey would be feasible and rewarding. We detected three distinct layers of 12CO(3–2) emission, related to the Cygnus Rift (500–800 pc), to W75N (1–1.8 kpc), and to DR 21 (1.5–2.5 kpc). Within the Cygnus Rift, H i self-absorption features are tightly correlated with faint diffuse CO emission, while HISA features in the DR 21 layer are mostly unrelated to any CO emission. 47 molecular outflows were detected in the pathfinder, 27 of them previously unknown. Sequentially triggered star formation is a widespread phenomenon.
Publication date
AffiliationNational Science Infrastructure; National Research Council Canada
Peer reviewedYes
NPARC number21268992
Export citationExport as RIS
Report a correctionReport a correction
Record identifier098093d5-c076-4d9c-8898-c4c88183985d
Record created2013-11-29
Record modified2016-05-09
Bookmark and share
  • Share this page with Facebook (Opens in a new window)
  • Share this page with Twitter (Opens in a new window)
  • Share this page with Google+ (Opens in a new window)
  • Share this page with Delicious (Opens in a new window)