globule blanc - meaning and definition. What is globule blanc
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What (who) is globule blanc - definition

ISOLATED AND RELATIVELY SMALL DARK NEBULAE
Bok globules; Bok Globules; Bok Globule; Cometary globule

André Blanc         
ASSOCIATION FOOTBALL PLAYER
Andre Blanc (trainer); André Blanc (trainer); Andre Blanc
André Blanc was a physiotherapist who became manager of Olympique de Marseille for the 1942-43 season. He won the Coupe de France in this season.
Hippolyte Blanc         
  • Christ Church Episcopal, Morningside (1875-78), Blanc's first competition-winning design
  • Mayfield Free Church (1876-79), now [[Mayfield Salisbury Church]]
  • The massive Coats Memorial Baptist Church in Paisley
  • Detail on Coats Memorial Church in Paisley
  • Hippolyte Blanc's grave, Warriston Cemetery
BRITISH ARCHITECT
Hippolyte G Blanc; Hippolyte J Blanc
Hippolyte Jean Blanc (18 August 1844 – 17 March 1917) was a Scottish architect. Best known for his church buildings in the Gothic revival style, Blanc was also a keen antiquarian who oversaw meticulously researched restoration projects.
Martine Blanc         
  • Martine Blanc-Rérat
FRENCH AUTHOR AND ILLUSTRATOR OF BOOKS FOR CHILDREN
Martine Blanc-Rérat; Martine Blanc-Rerat; Martine Rérat; Martine Rerat; Martine Blanc Rérat; Martine Blanc Rerat
Martine Blanc (born 16 September 1944 in Clermont-Ferrand, Puy-de-Dôme) is a French author and illustrator of ten books for children including The story of Timothy, the Two Hoots series in collaboration with Helen Cresswell, and All about Jesus.

Wikipedia

Bok globule

In astronomy, Bok globules are isolated and relatively small dark nebulae, containing dense cosmic dust and gas from which star formation may take place. Bok globules are found within H II regions, and typically have a mass of about 2 to 50 solar masses contained within a region about a light year or so across (about 4.5×1047 m3). They contain molecular hydrogen (H2), carbon oxides and helium, and around 1% (by mass) silicate dust. Bok globules most commonly result in the formation of double- or multiple-star systems.