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- W2080669874 abstract "We surveyed the CO(1–0) transition in 16 regions at Galactic latitudes >45° which contain compact dust cores less than half a degree in size with E(B − V) values ∼ 0.1 mag. We discovered three new intermediate-velocity molecular clouds and two high-latitude molecular clouds with more typical local standard of rest velocity (∼0 km s−1). The three intermediate-velocity molecular clouds (detected in CO emission in 11 lines of sight) nearly double the number of previously known, CO-emitting clouds. In order to detect the CO(1–0) line, N(H2) values of at least 1019 cm−2 are necessary, implying that the molecular/atomic fraction of these objects is significant and is in contrast to the primarily atomic lines of sight with log N(H2) < 17.3 detected in absorption by FUSE. The three molecular clouds are projected on and likely associated with a previously known intermediate-velocity H i feature known as the Intermediate Velocity Spur that may extend to the Galactic halo." @default.
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- W2080669874 date "2010-10-04" @default.
- W2080669874 modified "2023-09-25" @default.
- W2080669874 title "INTERMEDIATE-VELOCITY MOLECULAR GAS AT HIGH NORTHERN GALACTIC LATITUDES" @default.
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