Document Type
Article
Publication Date
1-1-2013
Abstract
Herschel far-infrared imaging observations have revealed the density structure of the interface between H ii regions and molecular clouds in great detail. In particular, pillars and globules are present in many high-mass star-forming regions, such as the Eagle nebula (M 16) and the Rosette molecular cloud, and understanding their origin will help characterize triggered star formation.
Digital Commons Citation
Tremblin, P.; Minier, V.; Schneider, N.; and Anderson, L. D., "Pillars And Globules At The Edges Of H Ii Regions: Confronting Herschel Observations And Numerical Simulations" (2013). Faculty & Staff Scholarship. 932.
https://researchrepository.wvu.edu/faculty_publications/932
Source Citation
Tremblin, P., Minier, V., Schneider, N., Anderson, L. D. (2013). Pillars And Globules At The Edges Of H Ii Regions: Confronting Herschel Observations And Numerical Simulations. Astronomy and Astrophysics, 560, A19. http://doi.org/10.1051/0004-6361/201322233