activity
20182022
most citedThe CARMA-NRO Orion Survey: The filamentary structure as seen in CO emission

70 citations · 184 across the 8 of their papers we have counts for

collaborators

10 papers

astro-ph.GA202110 cited

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…

astro-ph.GA2021

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…

astro-ph.GA202123 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.GA202010 cited

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…

astro-ph.GA202028 cited

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…

astro-ph.SR2020

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…