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SMA millimeter observations of hot molecular cores

Universidad de Chile. Repositorio Académico

 
Título SMA millimeter observations of hot molecular cores
 
Autor Kurtz, Stan
Hernández-Hernández, Vicente
Zapata, Luis
Garay Brignardello, Guido Alejandro
 
Tema ISM: molecules
 
Descripción Artículo de Publicación ISI.
We present Submillimeter Array observations in the 1.3 mm continuum and the CH3CN (12K–11K) line of 17 hot
molecular cores associated with young high-mass stars. The angular resolution of the observations ranges from 1.
0
to 4.
0. The continuum observations reveal large (>3500 AU) dusty structures with gas masses from 7 to 375 M ,
which probably surround multiple young stars. The CH3CN line emission is detected toward all the molecular
cores at least up to the K = 6 component and is mostly associated with the emission peaks of the dusty objects.
We used the multiple K-components of the CH3CN and both the rotational diagram method and a simultaneous
synthetic local thermodynamic equilibrium model with the XCLASS program to estimate the temperatures and
column densities of the cores. For all sources, we obtained reasonable fits from XCLASS by using a model that
combines two components: an extended and warm envelope and a compact hot core of molecular gas, suggesting
internal heating by recently formed massive stars. The rotational temperatures lie in the range of 40–132 K and
122–485 K for the extended and compact components, respectively. From the continuum and CH3CN results, we
infer fractional abundances from 10−9 to 10−7 toward the compact inner components, which increase with the
rotational temperature. Our results agree with a chemical scenario in which the CH3CN molecule is efficiently
formed in the gas phase above 100–300 K, and its abundance increases with temperature.
 
Fecha 2014-09-23T13:28:32Z
2015-03-13T13:01:21Z
2014-09-23T13:28:32Z
2015-03-13T13:01:21Z
2014-05-07
 
Tipo Artículo de revista
 
Enlace The Astrophysical Journal, 786:38 (17pp), 2014 May 1
doi:10.1088/0004-637X/786/1/38
http://repositorio.uchile.cl/handle/2250/126476
 
Idioma en_US
 
Publicador The American Astronomical Society