Evolution of Density Perturbations in a Cylindrical Molecular Cloud Using Smoothed Particle Hydrodynamics

Molecular clouds have a hierarchical structure from few tens of parsecs for giants to few tenth of a parsec for proto-stellar cores. Nowadays, our observational techniques are so advanced that it has become possible to detect the small-scale substructures inside the molecular cores. The question th...

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Bibliographic Details
Main Authors: Nejad-Asghar, M., Soltani, J.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2009-12-01
Series:Serbian Astronomical Journal
Subjects:
Online Access:http://saj.matf.bg.ac.rs/179/pdf/061-067.pdf