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An Optical Polarization Study of the Bok Globule B361

Published online by Cambridge University Press:  04 August 2017

Munezo Seki  and
Tatsuhiko Hasegawa
Munezo Seki
Affiliation:
Astronomical Institute, Tohoku University, Sendai 980, Japan
Tatsuhiko Hasegawa
Affiliation:
Astronomical Institute, Tohoku University, Sendai 980, Japan

Extract

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B361 is an isolated, round-shaped globule in Cygnus. The results of FIR observations by Keene (1981) indicate that there are no internal heat sources while recent CO observations (Hirano et al. 1987) afford evidence for the existence of a few fragments in the core of the globule.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 82 - 84
Copyright
Copyright © Reidel 1987 

References

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