other query
modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Help |

C.D.S. - SIMBAD4 rel 1.7 - 2019.12.16CET14:13:53 |

**
2014A&A...565A..24F -
**
*
Astronomy and Astrophysics, volume 565A, 24-24 (2014/5-1)
*

* *

**
On the probability distribution function of the mass surface density of molecular clouds. I.
**

*
FISCHERA J.
*

**
Abstract (from CDS):
**

The probability distribution function (PDF) of the mass surface density is an essential characteristic of the structure of molecular clouds or the interstellar medium in general. Observations of the PDF of molecular clouds indicate a composition of a broad distribution around the maximum and a decreasing tail at high mass surface densities. The first component is attributed to the random distribution of gas which is modeled using a log-normal function while the second component is attributed to condensed structures modeled using a simple power-law. The aim of this paper is to provide an analytical model of the PDF of condensed structures which can be used by observers to extract information about the condensations. The condensed structures are considered to be either spheres or cylinders with a truncated radial density profile at cloud radius r_{cl}. The assumed profile is of the form ρ(r)=ρ_{c}/(1+(r/r_{0})^{2})^{n/2} for arbitrary power n where ρ_{c} and r_{0} are the central density and the inner radius, respectively. An implicit function is obtained which either truncates (sphere) or has a pole (cylinder) at maximal mass surface density. The PDF of spherical condensations and the asymptotic PDF of cylinders in the limit of infinite overdensity ρ_{c}/ρ(r_{cl}) flattens for steeper density profiles and has a power law asymptote at low and high mass surface densities and a well defined maximum. The power index of the asymptote Σ^{–γ} of the logarithmic PDF (ΣP(Σ)) in the limit of high mass surface densities is given by γ=(n+1)/(n-1)-1 (spheres) or by γ=n/(n-1)-1 (cylinders in the limit of infinite overdensity).

**
Abstract Copyright:
**
∼

**
Journal keyword(s):
**
*
ISM: clouds - ISM: structure - methods: analytical - methods: statistical
*

**
Simbad objects:
**
4

Number of rows : 4 |

N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2020 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|

1 | NAME Taurus Dark Cloud | SFR | 04 41.0 | +25 52 | ~ | 3339 | 0 | |||||

2 | NAME ROSETTE MOL CLOUD | MoC | 06 34.7 | +04 02 | ~ | 224 | 0 | |||||

3 | NAME Coalsack Nebula | DNe | 12 31 19 | -63 44.6 | ~ | 239 | 0 | |||||

4 | NAME Lupus V | MoC | 16 21 | -37.5 | ~ | 52 | 0 |

To bookmark this query, right click on this link: simbad:objects in 2014A&A...565A..24F and select 'bookmark this link' or equivalent in the popup menu

2019.12.16-14:13:53

© Université de Strasbourg/CNRS

• Contact