Hostname: page-component-f554764f5-44mx8 Total loading time: 0 Render date: 2025-04-22T20:40:58.905Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Chandrasekhar, S.: 1960, Radiative Transfer, (Dover), p. 29.Google Scholar
Davis, L., and Greenstein, J.: 1951, Astrophys. J. 114, 206.Google Scholar
Gottlieb, D.M.: 1978, Astrophys. J. Suppl. 38, 287.CrossRefGoogle Scholar
Hirano, N., Hasegawa, T., Kameya, O., Takakubo, K., and Seki, M.: 1987, in Star Forming Regions (IAU Symposium 115, Reidel).Google Scholar
Keene, J.: 1981, Astrophys. J. 245, 115.CrossRefGoogle Scholar
Schmidt, E.G.: 1975, Month. Notices Roy. Astron. Soc. 172, 401.Google Scholar
Vallee, J.P.: 1983, Astron. Astrophys. 124, 147.Google Scholar