Buscar
Mostrando ítems 31-40 de 2159
Modelling [C I] emission from turbulent molecular clouds
(Royal Astronomical Society, 2015)
We use detailed numerical simulations of a turbulent molecular cloud to study the usefulness
of the [CI] 609 and 370 μmfine structure emission lines as tracers of cloud structure. Emission
from these lines is observed ...
Physical properties of molecular clouds in the southern outer Galaxy
(1997)
We have used a deep CO survey of the third galactic quadrant (May et al. 1993) to derive the physical properties of molecular clouds in the outer Galaxy. Within the range of this survey, from 194° to 270° in galactic ...
SuperMALT: Physical and Chemical Properties of Massive and Dense Clumps
(Cambridge University Press, 2017)
The SuperMALT survey is observing 76 MALT90 clumps at different evolutionary stages (from pre-stellar or quiescent to HII) in high excitation molecular lines and key isotopomers using the Apex 12m telescope with an angular ...
Investigation of the Large-scale Neutral Hydrogen near the Supernova Remnant W28
(IOP Publishing, 2002-10)
The distribution and kinematics of neutral hydrogen have been studied in a wide area around the supernova remnant (SNR) W28. A 2fdg5 × 2fdg5 field centered at l = 6fdg5, b = 0° was surveyed using the Parkes 64 m radio ...
IRAS 16547−4247: a new candidate of a protocluster unveiled with ALMA
(The American Astronomical Society, 2015-01-10)
We present the results of continuum and 12CO(3–2) and CH3OH(7–6) line observations of IRAS 16547−4247
made with the Atacama Large Millimeter/submillimeter Array (ALMA) at an angular resolution of ∼0.
5. The
12CO(3–2) ...