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most citedCompact starbursts in z~3-6 submillimeter galaxies revealed by ALMA

200 citations · 4.7k across the 136 of their papers we have counts for

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Showing 2014Show all

8 papers · 1 filter

astro-ph.GA2014

Molecular Gas and Star Formation in Voids

M. Das, T. Saito, D. Iono +2

We present the detection of molecular gas using CO(1-0) line emission and follow up Halpha imaging observations of galaxies located in nearby voids. The CO(1-0) observations were d…

astro-ph.GA2014★ 200 cited

Compact starbursts in z~3-6 submillimeter galaxies revealed by ALMA

Soh Ikarashi, R. J. Ivison, Karina I. Caputi +17

We report the source size distribution, as measured by ALMA millimetric continuum imaging, of a sample of 13 AzTEC-selected submillimeter galaxies (SMGs) at z_photo ~ 3-6. Their in…

astro-ph.GA2014★ 26 cited

Properties of Molecular Gas in Galaxies in Early and Mid Stage of Interaction: II. Molecular Gas Fraction

Hiroyuki Kaneko, Nario Kuno, Daisuke Iono +4

We have investigated properties of the interstellar medium in interacting galaxies in early and mid-stage using mapping data of 12CO(1-0) and HI.Assuming the standard CO-H2 convers…

astro-ph.GA2014★ 31 cited

Around the Ring We Go: The Cold, Dense Ring of Molecular Gas in NGC 1614

Kazimierz Sliwa, Christine D. Wilson, Daisuke Iono +2

We present high-resolution archival Atacama Large Millimeter/submillimeter Array (ALMA) CO J=3-2 and J=6-5 and HCO+ J=4-3 observations and new CARMA CO and 13CO J=1-0 observations…

astro-ph.GA2014★ 117 cited

Cold Molecular Gas in Merger Remnants: I. Formation of Molecular Gas Disks

Junko Ueda, Daisuke Iono, Min S. Yun +11

We present < 1 kpc resolution CO imaging study of 37 optically-selected local merger remnants using new and archival interferometric maps obtained with ALMA, CARMA, SMA and PdBI. W…

astro-ph.SR2014★ 79 cited

Cluster Formation Triggered by Filament Collisions in Serpens South

Fumitaka Nakamura, Koji Sugitani, Tomohiro Tanaka +24

The Serpens South infrared dark cloud consists of several filamentary ridges, some of which fragment into dense clumps. On the basis of CCS (), HCN (), N$_2…