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Outer-Galaxy molecular clouds

Published online by Cambridge University Press:  04 August 2017

Marc L. Kutner  and
Kathryn N. Mead
Marc L. Kutner
Affiliation:
Physics Department, Rensselaer Polytechnic Institute
Kathryn N. Mead
Affiliation:
Physics Department, Rensselaer Polytechnic Institute

Extract

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Since our original report of CO emission from outside the solar circle in the first quadrant (Kutner and Mead, 1981) we have extended the observations in two ways: (1) We have improved latitude and longitude coverage. Preliminary results on the latitude distribution were reported by Kutner (1983). (2) We have extended our cloud mapping, giving us at least partial CO maps of 55 clouds, along with 13CO, C18O, CO (2–1), and 2-mm H2CO observations of some clouds.

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Information
Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 209 - 210
Copyright
Copyright © Reidel 1985 

References

Blitz, K., Kulkarni, S., Heiles, C. 1981, BAAS, 13, 539 Google Scholar
Kutner, M.L., Mead, K.M. 1981, Ap. J. (Lett.), 267, L29 Google Scholar
Kutner, M.L. 1983, in “Southern Galactic Surveys”, eds. Burton, W.B. and Israel, F.P., Dordrecht: Reidel, 143 Google Scholar
Solomon, P.M., Stark, A.A., Sanders, D.B. 1983, Ap. J. (Lett.) 267, L29 Google Scholar