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An out-of-plane CO survey of the first galactic quadrant

Published online by Cambridge University Press:  14 August 2015

R. S. Cohen ,
G. R. Tomasevich  and
P. Thaddeus
R. S. Cohen
Affiliation:
NASA/Goddard Institute for Space Studies, New York City
G. R. Tomasevich
Affiliation:
NASA/Goddard Institute for Space Studies, New York City
P. Thaddeus
Affiliation:
NASA/Goddard Institute for Space Studies, New York City

Extract

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We are undertaking at Columbia University an out-of-plane survey of 2.6 mm CO emission from the first quadrant of the galactic disk with a 1.2 meter telescope. With the 8′ beamwidth of this instrument at 2.6 mm (about that of the largest existing steerable instruments at 21 cm) it is possible to completely map the first quadrant in only a few hundred days of observation.

Type
II. THE DISK COMPONENT
Information
Symposium - International Astronomical Union , Volume 84: The Large-Scale Characteristics of the Galaxy , 1979 , pp. 53 - 56
Copyright
Copyright © Reidel 1979 

References

Burton, W.B., and Shane, W.W.: 1970, in Becker, and Contopoulos, (eds.), The Spiral Structure of Our Galaxy, IAU Symposium No. 38, p. 397, D. Reidel, Dordrecht.Google Scholar
Burton, W.B., and Gordon, M.A.: 1978, Astron. Astrophys. 63, p. 7.Google Scholar
Cohen, R.S.: 1978, , , reprinted as NASA Technical Memorandum 78071, Goddard Space Flight Center, Greenbelt, MD.Google Scholar
Cohen, R.S., and Thaddeus, P.: 1977, Ap. J. Lett. 217, p. L155.Google Scholar
Scoville, N.Z., and Solomon, P.M.: 1975, Ap. J. Lett. 199, p. L105.Google Scholar
Shane, W.W.: 1972, Astron. Astrophys. 16, p. 118.Google Scholar