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20032009
most citedAzTEC Millimetre Survey of the COSMOS Field: I. Data Reduction and Source Catalogue

223 citations

Showing 2008 · astro-phShow all

6 papers · 2 filters

astro-ph200858 cited

AzTEC Millimetre Survey of the COSMOS Field - II. Source Count Overdensity and Correlations with Large-Scale Structure

J. E. Austermann, I. Aretxaga, D. H. Hughes +9

We report an over-density of bright sub-millimetre galaxies (SMGs) in the 0.15 sq. deg. AzTEC/COSMOS survey and a spatial correlation between the SMGs and the optical-IR galaxy den…

astro-ph200830 cited

Alignments of Group Galaxies with Neighboring Groups

Yougang Wang, Changbom Park, Xiaohu Yang +2

Using a sample of galaxy groups found in the Sloan Digital Sky Survey Data Release 4, we measure the following four types of alignment signals: (1) the alignment between the distri…

astro-ph20089 cited

Numerical Simulations of a Protostellar Outflow Colliding with a Dense Molecular Cloud

Chang Hyun Baek, Jongsoo Kim, Minho Choi

High-resolution SiO observations of the NGC 1333 IRAS 4A star-forming region showed a highly collimated outflow with a substantial deflection. The deflection was suggested to be ca…

astro-ph200833 cited

Computation of mass loss from viscous accretion disc in presence of cooling

Santabrata Das, Indranil Chattopadhyay

Rotating accretion flow may undergo centrifugal pressure mediated shock transition even in presence of various dissipative processes, such as viscosity and cooling mechanism. The e…

astro-ph2008223 cited

AzTEC Millimetre Survey of the COSMOS Field: I. Data Reduction and Source Catalogue

K. S. Scott, J. E. Austermann, T. A. Perera +10

We present a 1.1 mm wavelength imaging survey covering 0.3 sq. deg. in the COSMOS field. These data, obtained with the AzTEC continuum camera on the James Clerk Maxwell Telescope (…

astro-ph20086 cited

How was the mushroom-shaped GW 123.4--1.5 formed in the Galactic disk?

Chang Hyun Baek, Takahiro Kudoh, Kohji Tomisaka

The unusual mushroom-shaped HI cloud, GW 123.4--1.5, is hundreds of parsecs in size but does not show any correlations to HI shells or chimney structures. To investigate the origin…