The diffuse clouds towards Cyg OB2 No. 5 and No. 12
Journal article, 2005

We have investigated, in the 13CO(1-0) line, the region between the stars Cyg OB2 No. 5 and No, 12. The integrated intensity contour map reveals the existence of a condensation at 12 km s-1 (core C), north-west of Cyg OB2 No. 5, with a core-halo structure. The morphology and the derived physical parameters make it quite similar to core A, previously discovered towards Cyg OB2 No. 12. A second condensation at 7 km s -1, near Cyg OB2 No. 12, has been mapped in the same line (1-0) of 13CO. A summary of different observations, in all spectral regions, towards Cyg OB2 No. 5 and No. 12 is presented to provide the material for a further comprehensive discussion of this intricate and still intriguing region.

Author

S. Casu

Istituto nazionale di astrofisica (INAF)

F. Scappini

Istituto per lo Studio dei Materiali Nanostrutturati del C.N.R.

C. Cecchi-Pestellini

University of Salento

Michael Olberg

Chalmers, Department of Radio and Space Science

Monthly Notices of the Royal Astronomical Society

0035-8711 (ISSN) 1365-2966 (eISSN)

Vol. 359 1 73-78

Subject Categories

Aerospace Engineering

DOI

10.1111/j.1365-2966.2005.08873.x

More information

Latest update

9/15/2023