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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., ...
Filament intersections and cold dense cores in Orion A North
(Oxford University Press, 2020)
We studied the filament structures and cold dense cores in OMC-2,3 region in Orion A North molecular cloud using the high-resolution N2H+ (1-0) spectral cube observed with the Atacama Large Millimeter/Submillimeter Array ...
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 ...
Scaled up low-mass star formation in massive star-forming cores in the G333 giant molecular cloud
(Oxford Univ Press, 2016)
Three bright molecular line sources in G333 have recently been shown to exhibit signatures of infall. We describe amolecular line radiative transfer (RT) modelling process which is required to extract the infall signature ...
Magnetic field components analysis of the SCUPOL 850μm polarization data catalog
(Chicago, 2013)
We present an extensive analysis of the 850 μm polarization maps of the SCUBA Polarimeter Legacy (SCUPOL) Catalogue produced by Matthews et al., focusing exclusively on the molecular clouds and star-forming regions. For ...
Cloud scale ISM structure and star formation in M51
(IOP Publishing Ltd, 2017)
We compare the structure of molecular gas at 40 pc resolution to the ability of gas to form stars across the disk of the spiral galaxy M51. We break the PAWS survey into 370 pc and 1.1 kpc resolution elements, and within ...
Modelling [CI] emission from turbulent molecular clouds
(Oxford University Press, 2015)
© 2015 The Authors.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 ...
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 ...
Deuteration in infrared dark clouds
(Oxford University Press, 2016)
Much of the dense gas in molecular clouds has a filamentary structure but the detailed structure and evolution of this gas is poorly known. We have observed 54 cores in infrared dark clouds (IRDCs) using N2H+ (1-0) and ...