... molecules 1 Introduction Carbon monoxide is an effective tracer of molecularclouds ... profiles, which is often due to the clumpy structure of molecularclouds (Blitz 1991 ...
... resolved the molecular gas into a large number of compact clouds, with masses ... star clusters suggesting that individual molecularclouds are transformed in the ... star clusters from individual giant molecularclouds crushed by a sudden galactic ...
... the arms, but even these regions are hardly identified with giant molecularclouds ... find no giant HII regions at two giant molecularclouds located close to the center ...
... formed in the surface of the molecularcloud by ultraviolet radiation from the ... between the HII region and the molecularcloud; this has a thickness of about 10 -4 ...
... be a major component of interstellar molecularclouds, and the effects of the dust ... For interstellar molecularclouds this charge is negative (i.e., ). ... observed large widths of CO emission lines from molecularclouds (Arons and Max 1975 ...
... Mark Heyer "Magnetic Fields in MolecularClouds" . ... Paolo Padoan "Magnetic fields in molecularclouds" . ... Hua-bai Li "Anchoring Galactic Magnetic Fields in Turbulent MolecularClouds" . ...
... that the gas and dust in molecularclouds collapse to form a gravitationally-bound ... the formation of clumps in molecularclouds and disrupt any already-forming clumps ...
... occurs within the dense parts of molecularclouds and complexes and may proceed as a ... expected to proceed in dense molecularclouds either because of instabilities within ...
... A wide range of organic molecules have been detected in molecularclouds, but no amino acids. ... No chiral molecules have been detected in molecularclouds. ...
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... the front surface of the Lynds 1630 molecularcloud in Orion B (Depoy et al ... of emission from limb-brightened undulations in the surface of the molecularcloud ... interstellar value is incident on a clumpy molecularcloud, with the bulk of the gas ...