Buscar
Mostrando ítems 1-10 de 118
Kinematics of the Horsehead Nebula and IC 434 Ionization Front in CO and C+
(Institute of Physics Publishing, 2018)
The chemistry and kinematics of two molecular clouds near Sagittarius A*
(Oxford University Press, 2016)
We have analysed the chemical and kinematic properties of the 20 and 50 km s(-1) molecular clouds in the Central Molecular Zone of the Milky Way Galaxy, as well as those of the molecular ridge bridging these two clouds. ...
The Chemistry and Kinematics of Two Molecular Clouds near Sagittarius A
(Royal Astronomical Society, 2016-08-09)
We have analysed the chemical and kinematic properties of the 20 and 50 km s−1 molecular clouds in the Central Molecular Zone of the Milky Way Galaxy, as well as those of the molecular ridge bridging these two clouds. Our ...
Carbon-chain molecules in molecular outflows and Lupus I region – New producing region and new forming mechanism
(Oxford University Press, 2019)
GSH 91.5+2-114: A large H i shell in the outer part of the Galaxy
(EDP Sciences, 2011-01)
GSH 91.5 + 2 − 114 is a large H i shell located in the outer Galaxy at a kinematic distance of about 15 kpc. It was first identified in the Canadian Galactic Plane Survey (CGPS) by Pineault et al. (2002, ASP Conf. Ser., ...
Studying the kinematics of the giant star-forming region 30 Doradus
(EDP Sciences, 2013)
We present high-quality VLT-FLAMES optical spectroscopy of the nebular gas in the giant star-forming region 30 Doradus. In this
paper, the first of a series, we introduce our observations and discuss the main kinematic ...
EVOLUTION AND LIFETIME OF TRANSIENT CLUMPS IN THE TURBULENT INTERSTELLAR MEDIUM
(IOP PUBLISHING LTD, 2011)
We study the evolution of dense clumps and provide an argument that the existence of the clumps is not limited by their crossing times. We claim that the lifetimes of the clumps are determined by turbulent motions on a ...
Millimeter and far-IR study of the IRDC SDC 341.232-0.268
(Universidad Nacional Autónoma de México, 2019-07)
We analyze the molecular gas and dust associated with the infrared dark cloud SDC 341.232-0.268 in order to investigate the characteristics and parameters of the gas, determine the evolutionary status of four embedded EGO ...
The diffuse molecular component in the nuclear bulge of the Milky Way
(EDP Sciences, 2018)
Context. The bulk of the molecular gas in the central molecular zone (CMZ) of the Galactic center region shows warm kinetic temperatures, ranging from > 20 K in the coldest and densest regions (n similar to 10(4-5) cm(-3)) ...