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19992026
most citedThe Formation of Massive Stars from Turbulent Cores

1k citations · 9.5k across the 253 of their papers we have counts for

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Showing 2018Show all

13 papers · 1 filter

astro-ph.GA2018★ 21 cited

Multicomponent kinematics in a massive filamentary IRDC

Vlas Sokolov, Ke Wang, Jaime E. Pineda +6

To probe the initial conditions for high-mass star and cluster formation, we investigate the properties of dense filaments within the infrared dark cloud G035.39-00.33 (IRDC G035.3…

astro-ph.GA2018★ 41 cited

An Ordered Envelope-disk Transition in the Massive Protostellar Source G339.88-1.26

Yichen Zhang, Jonathan C. Tan, Nami Sakai +7

We report molecular line observations of the massive protostellar source G339.88-1.26 with the Atacama Large Millimeter/Submillimeter Array. The observations reveal a highly collim…

astro-ph.SR2018★ 16 cited

Disk wind feedback from high-mass protostars

Jan E. Staff, Kei E. I. Tanaka, Jonathan C. Tan

We perform a sequence of 3D magnetohydrodynamic (MHD) simulations of the outflow-core interaction for a massive protostar forming via collapse of an initial cloud core of $60~{M_\o…

astro-ph.SR2018★ 21 cited

IN-SYNC. VIII. Primordial Disk Frequencies in NGC 1333, IC 348, and the Orion A Molecular Cloud

Yuhan Yao, Michael R. Meyer, Kevin R. Covey +2

In this paper, we address two issues related to primordial disk evolution in three clusters (NGC 1333, IC 348, and Orion A) observed by the INfrared Spectra of Young Nebulous Clust…

astro-ph.GA2018★ 5 cited

High spectral resolution observations toward Orion BN at 6 m: no evidence for hot water

Nick Indriolo, Jonathan C. Tan, A. C. A. Boogert +4

Orion BN has a large proper motion and radial velocity with respect to the gas and other stars in the region where it is presumed to have formed. Multiple dynamical interaction sce…

astro-ph.GA2018★ 22 cited

Star Cluster Formation from Turbulent Clumps. II. Gradual Star Cluster Formation

Juan P. Farias, Jonathan C. Tan, Sourav Chatterjee

We investigate the dynamical evolution of star clusters during their formation, assuming that they are born from a turbulent starless clump of a given mass that is embedded within…