Filamentary Structure
Filamentary Structure is a morphological feature in the interstellar medium characterized by elongated, thread-like configurations of gas and dust that emerge from gravitational instabilities and turbulence in star-forming regions, serving as privileged sites for the formation of dense cores and protostellar systems within the large-scale structure of molecular clouds.
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How filaments of galaxies are woven into the cosmic web
J. Richard Bond, Lev Kofman, Dmitry Pogosyan · Nature · 1996 · 1.1K citations · Full text
Natural Sciences, Astronomy, Physics +12
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Centre National de la Recherche Scientifique
Paris, France
77 h-index
1.2K publications
173K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
60 h-index
318 publications
26.9K citations
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
56 h-index
479 publications
90.6K citations
CEA Paris-Saclay
Gif-sur-Yvette, France
51 h-index
393 publications
75.1K citations
Université Paris Cité
Paris, France
50 h-index
420 publications
86.9K citations
California Institute of Technology
Pasadena, United States
48 h-index
209 publications
29.6K citations
Astrophysique, Instrumentation et Modélisation
Gif-sur-Yvette, France
47 h-index
359 publications
79.2K citations
Institut de Recherche sur les Lois Fondamentales de l'Univers
Gif-sur-Yvette, France
46 h-index
299 publications
76.5K citations
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ApJ · 546 publications · 49.9K citations
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PRL · 48 publications · 3.5K citations
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AJ · 50 publications · 3.4K citations
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