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CO Observations of B361 and its Environment

Published online by Cambridge University Press:  04 August 2017

N. Hirano ,
T. Hasegawa ,
O. Kameya ,
K. Takakubo  and
M. Seki
N. Hirano
Affiliation:
Astronomical Institute, Tohoku University, Sendai, Japan
T. Hasegawa
Affiliation:
Astronomical Institute, Tohoku University, Sendai, Japan
O. Kameya
Affiliation:
Astronomical Institute, Tohoku University, Sendai, Japan
K. Takakubo
Affiliation:
Astronomical Institute, Tohoku University, Sendai, Japan
M. Seki
Affiliation:
College of General Education, Tohoku University, Sendai, Japan

Extract

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Extensive mapping of the CO and 13CO (J = 1-0) emission of the Bok globule, B361, is reported. The observations were made with the 4-m millimeter-wave telescope of Nagoya University. The mapped area extends over 60'x40′ which includes some filamentary dark clouds: L967, L964, L961, and L960, located to the west of B361.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 76 - 78
Copyright
Copyright © Reidel 1987 

References

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