Characterizing filaments in regions of high-mass star formation: High-resolution submilimeter imaging of the massive star-forming complex NGC 6334 with ArTéMiS

André, Ph.; Revéret, V.; Könyves, V.; Arzoumanian, D.; Tigé, J.; Gallais, P.; Roussel, H.; Le Pennec, J.; F. Rodrı́guez, Luis; Doumayrou, E.; Dubreuil, Didier; Lortholary, Michel; Martignac, J.; Talvard, M.; Delisle, Colby; Visticot, François; Dumaye, Luc; De Breuck, C.; Shimajiri, Yoshito; Motte, F.; Bontemps, S.; Hennemann, M.; Zavagno, A.; Russeil, D.; Schneider, N.; Palmeirim, P.; Peretto, N.; Hill, T.; Minier, V.; Lara A., R.; L. J. Rygl, K.

doi:10.1051/0004-6361/201628378

Public

Characterizing filaments in regions of high-mass star formation: High-resolution submilimeter imaging of the massive star-forming complex NGC 6334 with ArTéMiS

Shared by NobleBlocks on May 27, 2016 • 12:00 AM UTC

Authors:

Ph. André

V. Revéret

V. Könyves

Abstract

Context. Herschel observations of nearby molecular clouds suggest that interstellar filaments and prestellar cores represent two fundamental steps in the star formation process. The observations support a picture of low-mass star formation according to which filaments of ~0.1 pc width form first in ...

Subject

Physics

Star formation

Astrophysics

Research Assistant

AI chat, annotations, notes & similar papers

Finding related papers...

Discussions

(0)

No comments yet

Be the first to share your thoughts!