21 to 30 of 45 Results
Sep 5, 2016 -
ATLASGAL Extended Observations: Continuum (2D)
Adobe PDF - 29.8 KB -
MD5: 3b56c66ccf1c29aed9ac5e9b24c400d1
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Sep 5, 2016 -
ATLASGAL Catalogs: Source-Based Lists
Adobe PDF - 28.4 KB -
MD5: 754d0d74c92e25f7cd17e9a12e17634e
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Sep 5, 2016
The APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) maps 400 sq. deg. of the inner galaxy (|l| < 60º, |b| < 1.5º) at 870 μm with a uniform sensitivity of a few solar masses at a distance of 1 kpc. It has a spatial resolution of 19”. Its main sciences goals are to understand the early stages of high mass star formation, through a comprehen... |
Sep 5, 2016 -
COHRS Extended Observations: Spectral Line (3D)
Adobe PDF - 31.2 KB -
MD5: 2212486e7b71255f90de60b676e9e787
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Sep 5, 2016
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... |
Sep 5, 2016 -
CHIMPS Extended Observations: Spectral Line (3D)
Adobe PDF - 32.6 KB -
MD5: 1944a328e77a34875fa0e54c913c1086
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Sep 5, 2016
The 13CO/C18O (J = 3 → 2) Heterodyne Inner Milky Way Plane Survey (CHIMPS) is a high-resolution spectral survey covering |b| ≤ 0.5° and 28° ≲ l ≲ 46°. It has an angular resolution of 15” and consists of 0.5 km/s velocity channels. Because of its rarer isotopologues the survey probes a higher critical density of CO (>10^4 cm^-3) at temperatures less... |
Sep 5, 2016 -
BGPS Extended Observations: Continuum (2D)
Adobe PDF - 29.0 KB -
MD5: dff195431caf875417f8185bbd5e6639
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Sep 5, 2016 -
BGPS Catalogs: Source-Based Lists
Adobe PDF - 32.1 KB -
MD5: ff2ce81089a7d097563a245b9b97cab6
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Sep 5, 2016 -
BGPS Catalogs: Spectral Line
Adobe PDF - 31.7 KB -
MD5: 0fb998bf0ad76908d0157328460adadc
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