The CO High-Resolution Survey (COHRS) maps the 12CO (J = 3 → 2) transition in the Galactic plane, between |b| <= 0. 5° and 10° < l < 65°. It has a spatial resolution of 16” and a velocity resolution of 1 km/s. It is intended as a complement to the BGPS, ATLASGAL Hi-GAL, and JCMT surveys of the Galactic plane. The 12CO (J = 3 → 2) is a particularly good tracer of the warmer (10-50 K) material of moderate density (10^4 cm-3) around cores. It is also a good tracer of outflow activity, which should aid morphological studies of bubbles and filaments.
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COHRS Extended Observations: Spectral Line (3D)
COHRS Extended Observations: Spectral Line (3D)
Sep 5, 2016
Jessica Dempsey, 2016, "COHRS Extended Observations: Spectral Line (3D)", https://doi.org/10.7910/DVN/Q44Y7K, Harvard Dataverse, V1
This dataset consists of extended, high-resolution spectral line observations in the 12CO (J = 3 → 2) transition towards the first Galactic quadrant of the Milky Way. Data products available include reduced (l,b,v) cubes, integrated intensity maps, and position-velocity maps. All are available for download at the CANFAR data archive here.
COHRS_Spectral_Data_Access.pdf
COHRS_Spectral_Data_Access.pdf
Sep 5, 2016 - COHRS Extended Observations: Spectral Line (3D)
Adobe PDF - 31.2 KB - MD5: 2212486e7b71255f90de60b676e9e787
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