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CO Observations of Draco Clouds, Unusual High Latitude Clouds

Published online by Cambridge University Press:  04 August 2017

Y. Ohashi ,
Y. Fukui  and
T. Iwata
Y. Ohashi
Affiliation:
Nagoya University, Japan
Y. Fukui
Affiliation:
Nagoya University, Japan
T. Iwata
Affiliation:
Nagoya University, Japan

Extract

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Due to highly sensitive detectors and to the observers' efforts the observations of high galactic latitude clouds (HLC) have been improved in the last few years. The detection of infrared cirrus clouds, which were discovered by the IRAS (Low et al. 1984), strongly stimulated research on HLC. It is generally considered that HLC are small clouds which lie around 100 pc of the Sun (Blitz et al. 1984). This idea is consistent with their small velocity (VLSR) in the CO (λ = 2.6 mm) line.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 80 - 81
Copyright
Copyright © Reidel 1987