88 citations · 366 across the 16 of their papers we have counts for
17 papers
Filament Formation via Collision-induced Magnetic Reconnection -- Kinematic Features
Shuo Kong, Griselda Arroyo-Chávez, Volker Ossenkopf-Okada +4
The Collision-induced Magnetic Reconnection (CMR) mechanism has recently been proposed as a filament formation model that emphasizes the active role of magnetic fields. To enable b…
CMR exploration II -- filament identification with machine learning
Duo Xu, Shuo Kong, Avichal Kaul +2
We adopt magnetohydrodynamics (MHD) simulations that model the formation of filamentary molecular clouds via the collision-induced magnetic reconnection (CMR) mechanism under varyi…
CMR exploration I -- filament structure with synthetic observations
Shuo Kong, Volker Ossenkopf-Okada, Héctor G. Arce +2
In this paper, we carry out a pilot parameter exploration for the collision-induced magnetic reconnection (CMR) mechanism that forms filamentary molecular clouds. Following Kong et…
Ionized carbon as a tracer of the assembly of interstellar clouds
Nicola Schneider, Lars Bonne, Sylvain Bontemps +9
Molecular hydrogen clouds are a key component of the interstellar medium because they are the birthplaces for stars. They are embedded in atomic gas that pervades the interstellar…
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,…
HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules -- I. Survey description and a first look toward W3(OH), W3 IRS5 and NGC 7538 IRS1
A. M. Jacob, D. A. Neufeld, P. Schilke +22
The HyGAL SOFIA legacy program surveys six hydride molecules -- ArH+, OH+, H2O+, SH, OH, and CH -- and two atomic constituents -- C+ and O -- within the diffuse interstellar medium…
The link between gas and stars in the S254-S258 star-forming region
D. A. Ladeyschikov, M. S. Kirsanova, A. M. Sobolev +5
The paper aims to study relation between the distributions of the young stellar objects (YSOs) of different ages and the gas-dust constituents of the S254-S258 star-formation compl…
High-resolution CARMA Observation of Molecular Gas in the North America and Pelican Nebulae
Shuo Kong, Héctor G. Arce, John M. Carpenter +15
We present the first results from a CARMA high-resolution CO(1-0), CO(1-0), and CO(1-0) molecular line survey of the North America and Pelican (NAP) Nebulae. C…
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…
The CARMA-NRO Orion Survey: Filament Formation via Collision-Induced Magnetic Reconnection -- The Stick in Orion A
Shuo Kong, Volker Ossenkopf-Okada, Héctor G. Arce +13
A unique filament is identified in the {\it Herschel} maps of the Orion A giant molecular cloud. The filament, which, we name the Stick, is ruler-straight and at an early evolution…
The CARMA-NRO Orion Survey: Protostellar Outflows, Energetics, and Filamentary Alignment
Jesse R. Feddersen, Héctor G. Arce, Shuo Kong +7
We identify 45 protostellar outflows in CO maps of the Orion A giant molecular cloud from the CARMA-NRO Orion survey. Our sample includes 11 newly detected outflows. We measure the…
Star Cluster Formation in Orion A
Wanggi Lim, Fumitaka Nakamura, Benjamin Wu +9
We introduce new analysis methods for studying the star cluster formation processes in Orion A, especially examining the scenario of a cloud-cloud collision. We utilize the CARMA-N…
First detection of [13CII] in the Large Magellanic Cloud
Yoko Okada, Ronan Higgins, Volker Ossenkopf-Okada +3
[13CII] observations in several Galactic sources show that the fine-structure [12CII] emission is often optically thick (the optical depths around 1 to a few). The aim of our study…
The CARMA-NRO Orion Survey: Statistical Signatures of Feedback in the Orion A Molecular Cloud
Jesse R. Feddersen, Héctor G. Arce, Shuo Kong +2
We investigate the relationship between turbulence and feedback in the Orion A molecular cloud using maps of CO(1-0), CO(1-0) and CO(1-0) from the CARMA-NRO Or…
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…
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…
The first CO+ image: Probing the HI/H2 layer around the ultracompact HII region Mon R2
S. P. Trevino-Morales, A. Fuente, A. Sanchez-Monge +12
The CO+ reactive ion is thought to be a tracer of the boundary between a HII region and the hot molecular gas. In this study, we present the spatial distribution of the CO+ rotatio…