Showing 2014 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2014★ 15 cited

Tracing H2 column density with atomic carbon (CI) and CO isotopologues

N. Lo, M. R. Cunningham, P. A. Jones +6

We present first results of neutral carbon ([CI], 3P1 - 3P0 at 492 GHz) and carbon monoxide (13CO, J = 1 - 0) mapping in the Vela Molecular Ridge cloud C (VMR-C) and G333 giant mol…

astro-ph.GA2014★ 20 cited

ASTE observations in the 345 GHz window towards the HII region N113 of the Large Magellanic Cloud

S. Paron, M. E. Ortega, M. Cunningham +4

N113 is an HII region located in the central part of the Large Magellanic Cloud (LMC) with an associated molecular cloud very rich in molecular species. Most of the previously obse…

astro-ph.GA2014★ 15 cited

New detections of HCN toward hot cores associated with 6.7 GHz methanol masers

Claire-Elise Green, James A. Green, Michael G. Burton +6

We present new detections of cyanodiacetylene (HCN) toward hot molecular cores, observed with the Tidbinbilla 34 m radio telescope (DSS-34). In a sample of 79 hot molecular c…

astro-ph.GA2014★ 8 cited

Molecular line mapping of the giant molecular cloud associated with RCW 106 - IV. Ammonia towards dust emission

Vicki Lowe, Maria R. Cunningham, James S. Urquhart +6

Here we report observations of the two lowest inversion transitions of ammonia with the 70-m Tidbinbilla radio telescope. They were conducted to determine the kinetic temperatures…

astro-ph.GA2014★ 1 cited

Shock Structure and Shock Heating in the Galactic Central Molecular Zone

Juergen Ott, Michael Burton, Paul Jones +1

We present maps of a large number of dense molecular gas tracers across the Central Molecular Zone of our Galaxy. The data were taken with the CSIRO/CASS Mopra telescope in Large P…

astro-ph.GA2014★ 11 cited

The Carbon Inventory in a Quiescent, Filamentary Molecular Cloud in G328

Michael Burton, Michael Ashley, Catherine Braiding +6

We present spectral line images of [CI] 809 GHz, CO J=1-0 115 GHz and HI 1.4 GHz line emission, and calculate the corresponding C, CO and H column densities, for a sinuous, quiesce…