Search Results - "Offner, Stella S. R."
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The Effects of Radiative Transfer on Low-Mass Star Formation
Published in The Astrophysical journal (20-09-2009)“…Forming stars emit a substantial amount of radiation into their natal environment. We use ORION, an adaptive mesh refinement (AMR) three-dimensional…”
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2
Formation of Massive Star Systems by Accretion
Published in Science (American Association for the Advancement of Science) (06-02-2009)“…Massive stars produce so much light that the radiation pressure they exert on the gas and dust around them is stronger than their gravitational attraction, a…”
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The formation of a quadruple star system with wide separation
Published in Nature (London) (12-02-2015)“…Observations of a wide-separation quadruple system in the Perseus star-forming region reveal a young protostar and three gravitationally bound dense gas…”
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Driven and Decaying Turbulence Simulations of Low-Mass Star Formation: From Clumps to Cores to Protostars
Published in The Astrophysical journal (20-10-2008)“…Molecular clouds are observed to be turbulent, but the origin of this turbulence is not well understood. As a result, there are two different approaches to…”
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Impact of Protostellar Outflows on Turbulence and Star Formation Efficiency in Magnetized Dense Cores
Published in The Astrophysical journal (01-10-2017)“…The star-forming efficiency of dense gas is thought to be set within cores by outflow and radiative feedback. We use magnetohydrodynamic simulations to…”
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STARFORGE: the effects of protostellar outflows on the IMF
Published in Monthly notices of the Royal Astronomical Society (01-04-2021)“…ABSTRACT The initial mass function (IMF) of stars is a key quantity affecting almost every field of astrophysics, yet it remains unclear what physical…”
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The Astrochemical Impact of Cosmic Rays in Protoclusters. I. Molecular Cloud Chemistry
Published in The Astrophysical journal (20-06-2019)“…We present astrochemical photodissociation region models in which cosmic-ray (CR) attenuation has been fully coupled to the chemical evolution of the gas. We…”
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The Formation and Evolution of Wide-orbit Stellar Multiples In Magnetized Clouds
Published in The Astrophysical journal (20-12-2019)“…Stars rarely form in isolation. Nearly half of the stars in the Milky Way have a companion, and this fraction increases in star-forming regions. However, why…”
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A Census of Outflow to Magnetic Field Orientations in Nearby Molecular Clouds
Published in The Astrophysical journal (01-12-2022)“…Abstract We define a sample of 200 protostellar outflows showing blue- and redshifted CO emission in the nearby molecular clouds Ophiuchus, Taurus, Perseus,…”
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10
Can magnetized turbulence set the mass scale of stars?
Published in Monthly notices of the Royal Astronomical Society (01-08-2020)“…ABSTRACT Understanding the evolution of self-gravitating, isothermal, magnetized gas is crucial for star formation, as these physical processes have been…”
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Evolution of giant molecular clouds across cosmic time
Published in Monthly notices of the Royal Astronomical Society (01-02-2020)“…ABSTRACT Giant molecular clouds (GMCs) are well studied in the local Universe, however, exactly how their properties vary during galaxy evolution is poorly…”
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Impact of Cosmic-Ray Feedback on Accretion and Chemistry in Circumstellar Disks
Published in The Astrophysical journal (01-10-2019)“…We use the gas-grain chemistry code uclchem to explore the impact of cosmic-ray feedback on the chemistry of circumstellar disks. We model the attenuation and…”
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13
Turbulence, coherence, and collapse: Three phases for core evolution
Published in Monthly notices of the Royal Astronomical Society (07-10-2022)“…ABSTRACT We study the formation, evolution, and collapse of dense cores by tracking structures in a magnetohydrodynamic simulation of a star-forming cloud. We…”
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An ALMA Search for Substructure and Fragmentation in Starless Cores in Orion B North
Published in The Astrophysical journal (01-06-2024)“…Abstract We present Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 3 observations of 73 starless and protostellar cores in the Orion B North…”
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The Formation of Low-mass Binary Star Systems Via Turbulent Fragmentation
Published in The Astrophysical journal (20-12-2010)“…We characterize the infall rate onto protostellar systems forming in self-gravitating radiation-hydrodynamics simulations. Using two dimensionless parameters…”
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Aluminum-26 Enrichment in the Surface of Protostellar Disks Due to Protostellar Cosmic Rays
Published in The Astrophysical journal (01-07-2020)“…The radioactive decay of aluminum-26 (26Al) is an important heating source in early planet formation. Since its discovery, there have been several mechanisms…”
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Coevolution of Stars and Gas: Using an Analysis of Synthetic Observations to Investigate the Star–Gas Correlation in STARFORGE
Published in The Astrophysical journal (01-12-2023)“…Abstract We explore the relation between stellar surface density and gas surface density (the star–gas, or S-G, correlation) in a 20,000 M ⊙ simulation from…”
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The Green Bank Ammonia Survey: First Results of NH3 Mapping of the Gould Belt
Published in The Astrophysical journal (01-07-2017)“…We present an overview of the first data release (DR1) and first-look science from the Green Bank Ammonia Survey (GAS). GAS is a Large Program at the Green…”
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Star-Gas Surface Density Correlations in 12 Nearby Molecular Clouds. I. Data Collection and Star-sampled Analysis
Published in The Astrophysical journal (01-06-2020)“…We explore the relation between the stellar mass surface density and the mass surface density of molecular hydrogen gas in 12 nearby molecular clouds that are…”
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An Episodic Wide-angle Outflow in HH 46/47
Published in The Astrophysical journal (20-09-2019)“…During star formation, the accretion disk drives fast MHD winds, which usually contain two components, a collimated jet and a radially distributed wide-angle…”
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