III. Probability distribution functions of molecular lines in Cygnus X

1) in greyscale. The black contour indicates the Av = 15 level. The red contours show the same Av = 15 level from the H2 column-density map derived from N2H+, ...

Star-forming clouds can best be characterised by lognormal PDFs for the lower N range and a power-law tail for higher N, which is commonly attributed to ...

Understanding star formation in molecular clouds. III. Probability ...

Understanding star formation in molecular clouds. III. Probability distribution functions of molecular lines in Cygnus X. Schneider, N. ;; Bontemps, S ...

[1509.01082] Understanding star formation in molecular clouds III ...

Title:Understanding star formation in molecular clouds III. Probability distribution functions of molecular lines in Cygnus X. Authors:N ...

Understanding star formation in molecular clouds: III. Probability ...

; Understanding star formation in molecular clouds: III. Probability distribution functions of molecular lines in Cygnus X. ; Schneider, N ; Bontemps, S ...

Understanding star formation in molecular clouds III. Probability ...

Understanding star formation in molecular clouds III. Probability distribution functions of molecular lines in Cygnus X. @article ...

Understanding star formation in molecular clouds III. Probability ...

Understanding star formation in molecular clouds III. Probability distribution functions of molecular lines in Cygnus X. September 2015 ...

Understanding star formation in molecular clouds-III. Probability ...

The probability distribution function of column density ... lines – converted into H 2 column density ... Cygnus X North region, and make a comparison to ...

Understanding star formatio... - Researchers - ANU

Understanding star formation in molecular clouds III. Probability distribution functions of molecular lines in Cygnus X. Citation. Schneider, N, Bontemps, S ...

What probability distribution functions tell us about the processes of ...

Related Articles · Understanding star formation in molecular clouds — III. Probability distribution functions of molecular lines in Cygnus X · Understanding star ...

Multilognormal density structure in Cygnus-X molecular clouds

We studied the H 2 column density probability distribution function (N-PDF) based on molecular emission lines using the Nobeyama 45-m Cygnus X CO survey data.

CO Mapping of Cygnus-X—Volume Density Distribution - IOPscience

We present CO(2-1) and 13 CO(2-1) maps of the Cygnus-X molecular cloud complex using the 10 m Heinrich Hertz Submillimeter Telescope.

[PDF] CO Mapping of Cygnus-X—Volume Density Distribution ...

CO Mapping of Cygnus-X—Volume Density Distribution ... Understanding star formation in molecular clouds III. Probability distribution functions of molecular lines ...

CO Mapping of Cygnus-X-Volume Density Distribution - NASA/ADS

We present CO(2-1) and 13 CO(2-1) maps of the Cygnus-X molecular cloud complex using the 10 m Heinrich Hertz Submillimeter Telescope.

Understanding star formation in molecular clouds - HAL

formation in molecular clouds: III. Probability distribution functions of molecular lines in Cygnus. X. Astronomy and Astrophysics - A&A ...

Multi log-normal density structure in cygnus-X molecular clouds

We studied the H2 column density probability distribution function (N-PDF) based on molecular emission lines using the Nobeyama 45-m Cygnus X CO survey data ...

arXiv:1509.01082v2 [astro-ph.GA] 15 Jan 2016

Understanding star formation in molecular clouds. III. Probability distribution functions of molecular lines in Cygnus X. N.Schneider1,2, S ...

Young and embedded clusters in Cygnus-X: evidence for building ...

Investigation of their mass distributions in low-mass domain revealed a relatively uniform log-normal initial mass function (IMF) with a characteristic mass of ...

List of Publications

Understanding star formation in molecular clouds. III. Probability distribution functions of molecular lines in Cygnus X A&A , 587; 74, 2016; Arshakian ...

Ionized carbon as a tracer of the assembly of interstellar clouds

Figure 1 shows the 12CO 1 → 0 and [CII] line integrated emission distribution in the three main velocity ranges in Cygnus X. These are ...