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20152025
most citedDisruption of the Orion Molecular Core 1 by the stellar wind of the massive star Ori C

140 citations · 1.3k across the 31 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

astro-ph.SR2019★ 53 cited

Chemical complexity in high-mass star formation: An observational and modeling case study of the AFGL 2591 VLA 3 hot core

C. Gieser, D. Semenov, H. Beuther +30

We present a detailed observational and modeling study of the hot core VLA 3 in the high-mass star-forming region AFGL 2591, which is a target region of the NOrthern Extended Milli…

astro-ph.SR2019★ 7 cited

The CARMA-NRO Orion Survey: Core Emergence and Kinematics in the Orion A Cloud

Shuo Kong, Héctor G. Arce, Anneila I. Sargent +19

We have investigated the formation and kinematics of sub-mm continuum cores in the Orion A molecular cloud. A comparison between sub-mm continuum and near infrared extinction shows…

astro-ph.GA2019★ 118 cited

Dynamics of cluster-forming hub-filament systems: The case of the high-mass star-forming complex Monoceros R2

S. P. Trevino-Morales, A. Fuente, A. Sanchez-Monge +15

High-mass stars and star clusters commonly form within hub-filament systems. Monoceros R2, harbors one of the closest such systems, making it an excellent target for case studies.…

astro-ph.SR2019★ 22 cited

IRAS23385+6053: An embedded massive cluster in the making

R. Cesaroni, H. Beuther, A. Ahmadi +26

This study is part of the project ``CORE'', an IRAM/NOEMA large program consisting of observations of the millimeter continuum and molecular line emission towards 20 selected high-…

astro-ph.GA2019★ 91 cited

The dynamical evolution of molecular clouds near the Galactic Centre - II. Spatial structure and kinematics of simulated clouds

J. M. D. Kruijssen, J. E. Dale, S. N. Longmore +16

The evolution of molecular clouds in galactic centres is thought to differ from that in galactic discs due to a significant influence of the external gravitational potential. We pr…

astro-ph.GA2019★ 140 cited

Disruption of the Orion Molecular Core 1 by the stellar wind of the massive star Ori C

C. Pabst, R. Higgins, J. R. Goicoechea +10

Massive stars inject mechanical and radiative energy into the surrounding environment, which stirs it up, heats the gas, produces cloud and intercloud phases in the interstellar me…