Universität zu Köln

Veltchev, Todor V., Ossenkopf-Okada, Volker, Stanchev, Orlin, Schneider, Nicola, Donkov, Sava and Klessen, Ralf S. (2018). Spatially associated clump populations in Rosette from CO and dust maps. Mon. Not. Roy. Astron. Soc., 475 (2). S. 2215 - 2236. OXFORD: OXFORD UNIV PRESS. ISSN 1365-2966

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Abstract

Spatial association of clumps from different tracers turns out to be a valuable tool to determine the physical properties of molecular clouds. It provides a reliable estimate for the X-factors, serves to trace the density of clumps seen in column densities only, and allows one to measure the velocity dispersion of clumps identified in dust emission. We study the spatial association between clump populations, extracted by use of the GAUSSCLUMPS technique from (CO)-C-12(1-0), (CO)-C-13(1-0) line maps and Herschel dust-emission maps of the star-forming region Rosette, and analyse their physical properties. All CO clumps that overlap with another CO or dust counterpart are found to be gravitationally bound and located in the massive star-forming filaments of the molecular cloud. They obey a single mass-size relation M-cl proportional to R-cl(gamma) with gamma similar or equal to 3 (implying constant mean density) and display virtually no velocity-size relation. We interpret their population as low-density structures formed through compression by converging flows and still not evolved under the influence of self-gravity. The high-mass parts of their clump mass functions are fitted by a power law dN(cl)/d log M-cl proportional to M-cl(Gamma) cl and display a nearly Salpeter slope Gamma similar to -1.3. On the other hand, clumps extracted from the dust-emission map exhibit a shallower mass-size relation with gamma = 2.5 and mass functions with very steep slopes Gamma similar to -2.3 even if associated with CO clumps. They trace density peaks of the associated CO clumps at scales of a few tenths of pc where no single density scaling law should be expected.

Item Type:	Journal Article
Creators:	Creators Email ORCID ORCID Put Code Veltchev, Todor V. UNSPECIFIED UNSPECIFIED UNSPECIFIED Ossenkopf-Okada, Volker UNSPECIFIED UNSPECIFIED UNSPECIFIED Stanchev, Orlin UNSPECIFIED UNSPECIFIED UNSPECIFIED Schneider, Nicola UNSPECIFIED UNSPECIFIED UNSPECIFIED Donkov, Sava UNSPECIFIED UNSPECIFIED UNSPECIFIED Klessen, Ralf S. UNSPECIFIED UNSPECIFIED UNSPECIFIED
URN:	urn:nbn:de:hbz:38-192120
DOI:	10.1093/mnras/stx3267
Journal or Publication Title:	Mon. Not. Roy. Astron. Soc.
Volume:	475
Number:	2
Page Range:	S. 2215 - 2236
Date:	2018
Publisher:	OXFORD UNIV PRESS
Place of Publication:	OXFORD
ISSN:	1365-2966
Language:	English
Faculty:	Unspecified
Divisions:	Unspecified
Subjects:	no entry
Uncontrolled Keywords:	Keywords Language MOLECULAR CLOUD; MASS FUNCTION; FRACTAL ORIGIN; CORES; EMISSION; DENSITY; LUMINOSITY; TURBULENCE; HERSCHEL; SPECTRUM Multiple languages Astronomy & Astrophysics Multiple languages
Refereed:	Yes
URI:	http://kups.ub.uni-koeln.de/id/eprint/19212