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54645 304..321and filaments in orion b brenda c. matthews jason d. fiege canadian institute for theoretical astrophysics, university of toronto, 60 saint george street, toronto,
c: the astrophysical journal, 738:101 (20pp), 2011 september 1 doi:10.1088/0004-637x/738/1/101 c© 2011. the american astronomical society. all rights reserved. printed
the dynamical evolution of molecular clouds near the galactic centre – ii. spatial structure and kinematics of simulated cloudsmnras 484, 5734–5754 (2019) doi:10.1093/mnras/stz381
mon not r astron soc 000 1– 3004 printed november 7 2018 mn latex style file v22 the simulation of molecular clouds formation in the milky way sa khoperskov1 eo vasiliev2…
34 chapter 3 molecular clouds notes: • most of the material presented in this chapter is taken from stahler and palla 2004 chap 3 31 definitions and preliminaries we mainly…
evolution of molecular clouds msevenster sterrewacht leiden the evolution of interstellar molecular hydrogen was studied with a special interest for the formation and evolution…
the life cycle of giant molecular clouds charlotte christensen observational constraints on the life cycle of giant molecular clouds in milky way-like galaxies charlotte…
magnetic field structure in molecular clouds by polarization measurements magnetic field structure in molecular clouds by polarization measurements wen-ping chen national…
star formation from (local) molecular clouds to spiral arms lee hartmann university of michigan structure of molecular clouds efficiency of star formation feedback mechanisms…
the structur and evolution of molecular clouds: from clumps to cores to the imf j.p.williams; l. blitz; c.f.mckee introduction molecular clouds are generally: self-gravitating,…
from filamentary networks to dense cores in molecular clouds: toward a new paradigm for star formation philippe andr é laboratoire d’astrophysique de paris-saclay james…
atmos. chem. phys., 13, 12343–12362, 2013 www.atmos-chem-phys.net/13/12343/2013/ doi:10.5194/acp-13-12343-2013 © author(s) 2013. cc attribution 3.0 license. atmospheric…
lecture4_ph6820fields in molecular clouds herschel image of the rosette cloud molecular cloud properties composition: h2, he, dust (1% mass), co (10-4 by number), and many
astronomy & astrophysics manuscript no. m33cprops c© eso 2018 august 27, 2018 giant molecular clouds in the local group galaxy m33 p. gratier1,2, j. braine1, n.j.
slide 1 the structur and evolution of molecular clouds: from clumps to cores to the imf j.p.williams; l. blitz; c.f.mckee 1.introduction molecular clouds are generally: self-gravitating,…
star formation in molecular clouds collaborators: ralf klessen (ita) ian bonnell (st andrews) hans zinnecker (aip) matthew bate (exeter) jim dale (leicester/ita) clare dobbs…
mnras 453 2036–2049 2015 doi:101093mnrasstv1750 filaments in the lupus molecular clouds m benedettini1‹ e schisano1‹ s pezzuto1 d elia1 p andré2 v könyves2 n schneider3…
giant molecular clouds in local group galaxies leo blitz university of california, berkeley yasuo fukui nagoya university akiko kawamura nagoya university adam leroy university…
tagging molecular clouds in turbulent air citation for published version apa: mirzaei, m. 2013. tagging molecular clouds in turbulent air. technische universiteit eindhoven.…
structure of turbulence intermittency in molecular clouds p hily-blant ipag atelier osug june 18th 2012 introduction structures dissipation questions references introduction…