activity
20142026
most citedThe CARMA-NRO Orion Survey

88 citations · 480 across the 21 of their papers we have counts for

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Showing astro-ph.GAShow all

16 papers · 1 filter

astro-ph.GA2026

ATT12: The Antarctic 12-m Terahertz Telescope for Studies of Dusty Galaxies. I. Instrument Sensitivity and Science Forecasts

Koki Wakasugi, Takuya Hashimoto, Nario Kuno +13

We present a feasibility study of the Antarctic 12m Terahertz Telescope (ATT12), a next-generation facility to be constructed at New Dome Fuji in Antarctica, designed to open up th…

astro-ph.GA2022★ 17 cited

ALMA Fragmented Source Catalogue in Orion (FraSCO) I. Outflow interaction within an embedded cluster in OMC-2/FIR3, FIR4, and FIR5

Asako Sato, Satoko Takahashi, Shun Ishii +6

We present a high angular resolution () and wide-field () image of the 1.3-mm continuum, CO( = 2--1) line, and SiO( = 5--4) line emissions toward an…

astro-ph.GA2022★ 16 cited

CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A

Hideaki Takemura, Fumitaka Nakamura, Héctor G. Arce +15

The mass distribution of dense cores is a potential key to understand the process of star formation. Applying dendrogram analysis to the CARMA-NRO Orion CO (=1--0) data,…

astro-ph.GA2021

Super-fast Rotation in the OMC 2/FIR 6b Jet

Yuko Matsushita, Satoko Takahashi, Shun Ishii +4

We present ALMA CO (=2--1) and 1.3 mm continuum observations of the high-velocity jet associated with the FIR 6b protostar located in the Orion Molecular Cloud-2. We detect a ve…

astro-ph.GA2021★ 6 cited

Atomic Carbon [CI] Mapping of the Nearby Galaxy M83

Yusuke Miyamoto, Atsushi Yasuda, Yoshimasa Watanabe +6

Atomic carbon (CI) has been proposed to be a global tracer of the molecular gas as a substitute for CO, however, its utility remains unproven. To evaluate the suitability of CI as…

astro-ph.GA2021★ 23 cited

The Core Mass Function in the Orion Nebula Cluster Region: What Determines the Final Stellar Masses?

Hideaki Takemura, Fumitaka Nakamura, Shuo Kong +29

Applying dendrogram analysis to the CARMA-NRO CO (=1--0) data having an angular resolution of 8", we identified 692 dense cores in the Orion Nebula Cluster (ONC) r…

astro-ph.GA2021★ 7 cited

The CO core mass function toward Orion A: Single-dish observations

Hideaki Takemura, Fumitaka Nakamura, Shun Ishii +6

We have performed an unbiased dense core survey toward the Orion A Giant Molecular Cloud in the CO (=1--0) emission line taken with the Nobeyama Radio Observatory (NRO) 4…

astro-ph.GA2019★ 35 cited

Nobeyama 45-m mapping observations toward nearby molecular clouds, Orion A, Aquila Rift, and M17: Project overview

Fumitaka Nakamura, Shun Ishii, Kazuhito Dobashi +16

We carried out mapping observations toward three nearby molecular clouds, Orion A, Aquila Rift, and M17, using a new 100 GHz receiver, FOREST, on the Nobeyama 45-m telescope. In th…

astro-ph.GA2019★ 24 cited

Nobeyama 45 m Mapping Observations toward Orion A. II. Classification of cloud structures and variation of the CO/CO abundance ratio due to far-UV Radiation

Shun Ishii, Fumitaka Nakamura, Yoshito Shimajiri +4

We present results of the classification of cloud structures toward the Orion A Giant Molecular Cloud based on wide-field CO ( = 1--0), CO ( = 1-0), and C$^{18}…

astro-ph.GA2019★ 70 cited

The CARMA-NRO Orion Survey: The filamentary structure as seen in CO emission

S. T. Suri, A. Sanchez-Monge, P. Schilke +18

We present an initial overview of the filamentary structure in the Orion A molecular cloud utilizing a high angular and velocity resolution CO(1-0) emission map that was rec…

astro-ph.GA2018★ 22 cited

Expanding CO Shells in the Orion A Molecular Cloud

Jesse R. Feddersen, Héctor G. Arce, Shuo Kong +6

We present the discovery of expanding spherical shells around low to intermediate-mass young stars in the Orion A giant molecular cloud using observations of CO (1-0) and $^…

astro-ph.GA2018★ 88 cited

The CARMA-NRO Orion Survey

Shuo Kong, Héctor G. Arce, Jesse R. Feddersen +35

We present the first results from a new, high resolution, CO(1-0), CO(1-0), and CO(1-0) molecular line survey of the Orion A cloud, hereafter referred to as th…

astro-ph.GA2018★ 20 cited

ALMA [CI] observations toward the central region of a Seyfert galaxy NGC 613

Yusuke Miyamoto, Masumichi Seta, Naomasa Nakai +3

We report ALMA observations of [CI](), CO, and CO () toward the central region of a nearby Seyfert galaxy NGC 613. The very high resolutions of $0…

astro-ph.GA2016★ 6 cited

A Multi-Line Ammonia Survey of the Galactic Center Region with the Tsukuba 32-m Telescope - I. Observations and Data

Hitoshi Arai, Makoto Nagai, Shinji Fujita +22

We present survey data of the NH3 (J, K) = (1, 1)--(6, 6) lines, simultaneously observed with the Tsukuba 32-m telescope, in the main part of the central molecular zone of the Gala…

astro-ph.GA2015★ 9 cited

Large-scale CO (J=4-3) Mapping toward the Orion-A Giant Molecular Cloud

Shun Ishii, Masumichi Seta, Makoto Nagai +10

We have mapped the Orion-A Giant Molecular Cloud in the CO (J=4-3) line with the Tsukuba 30-cm submillimeter telescope.The map covered a 7.125 deg^2 area with a 9' resolution, incl…

astro-ph.GA2014★ 13 cited

Hot Ammonia in the Center of the Seyfert 2 galaxy NGC 3079

Yusuke Miyamoto, Naomasa Nakai, Masumichi Seta +5

We present the results of ammonia observations toward the center of NGC 3079. The NH3(J, K) = (1, 1) and (2, 2) inversion lines were detected in absorption with the Tsukuba 32-m te…