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Bok globule

Bok globules dense, compact and cold interstellar clonds... [Pg.105]

Bok globule (a nebula from which a star is formed)... [Pg.252]

Launhardt R. and Sargent A. I. (2001) A young protoplanetary disk in the Bok globule CB 26 Astrophys. J. 562, L173-L175. [Pg.82]

Figure 14. Image of the HH 46/47 system arising from the Bok globule (ESO 210-6A) obtained with IRAC. The image covers a region of approximately 6.5 x 10.6 arcmin. Emission at 3.6, 4.5 and 5.8, and 8.0 /tm is shown as blue, green, and red, respectively. The inset is a visible light comparison image. Figure 14. Image of the HH 46/47 system arising from the Bok globule (ESO 210-6A) obtained with IRAC. The image covers a region of approximately 6.5 x 10.6 arcmin. Emission at 3.6, 4.5 and 5.8, and 8.0 /tm is shown as blue, green, and red, respectively. The inset is a visible light comparison image.
Stonier offers a novel explanation of the commonly observed dark (Bok) globules as approaching stellar objects, rather than contracting gas clouds, which occur in the early stages of star formation. He even has an explanation for the invisibility of Nemesis, the legendary companion of the sun. [Pg.270]

See other pages where Bok globule is mentioned: [Pg.113]    [Pg.102]    [Pg.113]    [Pg.102]   
See also in sourсe #XX -- [ Pg.105 , Pg.113 ]



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