Statistical link between the structure of molecular clouds and their density distribution
arXiv:1612.00340 · doi:10.1093/mnras/stw3147
Abstract
We introduce the concept of a class of equivalence of molecular clouds represented by an abstract spherically symmetric, isotropic object. This object is described by use of abstract scales in respect to a given mass density distribution. Mass and average density are ascribed to each scale and thus are linked to the density distribution: a power-law type and an arbitrary continuous one. In the latter case, we derive a differential relationship between the mean density at a given scale and the structure parameter which defines the mass-density relationship. The two-dimensional (2D) projection of the cloud along the line of sight is also investigated. Scaling relations of mass and mean density are derived in the considered cases of power-law and arbitrary continuous distributions. We obtain relations between scaling exponents in the 2D and 3D cases. The proposed classes of equivalence are representative for the general structure of real clouds with various types of column-density distributions: power law, lognormal or combination of both.
8 pages, 1 figure; accepted for publication in MNRAS
References in corpus (28)
- Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing
- The Statistics of Supersonic Isothermal Turbulence
- Probing the evolution of molecular cloud structure: From quiescence to birth
- On the Star Formation Efficiency of Turbulent Magnetized Clouds
- Molecular Cloud Evolution II. From cloud formation to the early stages of star formation in decaying conditions
- One-Point Probability Distribution Functions of Supersonic Turbulent Flows in Self-Gravitating Media
- Accretion-Driven Turbulence as Universal Process: Galaxies, Molecular Clouds, and Protostellar Disks
- On the Density Distribution in Star-forming Interstellar Clouds
- Gravity or Turbulence? The velocity dispersion-size relation
- Clump morphology and evolution in MHD simulations of molecular cloud formation
- On the Rapid Collapse and Evolution of Molecular Clouds
- On the evolution of the density pdf in strongly self-gravitating systems
- Unfolding the Laws of Star Formation: The Density Distribution of Molecular Clouds
- The Two States of Star Forming Clouds
- The link between molecular cloud structure and turbulence
- Molecular clouds have power-law probability distribution functions
- Six Myths on the Virial Theorem for Interstellar Clouds
- A Fractal Origin for the Mass Spectrum of Interstellar Clouds: II. Cloud Models and Power Law Slopes
- Understanding star formation in molecular clouds I. Effects of line-of-sight contamination on the column density structure
- Larson's third law and the universality of molecular cloud structure
- On the structure of molecular clouds
- Relationship between the column density distribution and evolutionary class of molecular clouds as viewed by ATLASGAL
- Stellar and substellar initial mass function: a model that implements gravoturbulent fragmentation and accretion
- Constructing multi-scale gravitational energy spectra from molecular cloud surface density PDF -- Interplay between turbulence and gravity
- Mass-density relationship in molecular cloud clumps
- The Stellar Initial Mass Function in 2007: A Year for Discovering Variations
- Clump mass function at an early stage of molecular cloud evolution: I. A statistical approach
- Clump mass function at an early stage of molecular cloud evolution: II. Galactic cloud complexes
Cited by in corpus (12)
- The shapes of column density PDFs - The importance of the last closed contour
- Density distribution function of a self-gravitating isothermal compressible turbulent fluid in the context of Molecular Clouds ensembles
- The relation between the true and observed fractal dimensions of turbulent clouds
- Dense Regions in Supersonic Isothermal Turbulence
- On the extraction of power-law parts of the probability density functions in star-forming clouds
- Fractal dimension of optical cirrus in Stripe82
- X-raying molecular clouds with a short flare: probing statistics of gas density and velocity fields
- Extraction of a second power-law tail of the density distribution in simulated clouds
- Density distribution function of a self-gravitating isothermal turbulent fluid in the context of molecular clouds ensembles -- III. Virial analysis
- Density profile of a self-gravitating polytropic turbulent fluid in a rotating disk near to the cloud core
- Statistical mass function of prestellar cores from the density distribution of their natal clouds
- Density profile of a self-gravitating polytropic turbulent fluid in the context of ensembles of molecular clouds