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An Intertextual Analysis of J i ́ mi S ̣ o ́ la n ́ k e ̣ ́ ’ s O ̣̀ n a L a (In The Path) via the Multiple Star System Theory of Mutual Illumination and Interaction
Published 2017-05-01“…Thus, drawing concepts from astrophysics, with specific reference to multiple star systems, a conceptual framework is derived in which analogous relations are proposed and interrogated. …”
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Formation of Massive and Wide First-star Binaries in Radiation Hydrodynamic Simulations
Published 2023-01-01“…We also identify such systems as mini-binaries embedded in a wider outer multiple-star system, which could evolve into progenitors for observed gravitational wave events.…”
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Search for a Black Hole Binary in Gaia DR3 Astrometric Binary Stars with Spectroscopic Data
Published 2023-01-01“…We argue that, if this dark object is not a BH, this system must be a more exotic system, in which the primary red giant branch star orbits around a quadruple star system (or a higher-order multiple-star system) whose total mass is more than 5.68 M _⊙ . …”
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The formation of binary stars
Published 2001“…Numerical simulations of this process do indicate that under certain conditions fragmentation does occur; however the simulations so far have not reached the point where they can explain the statistical properties of observed binary and multiple star systems.…”
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Triple Spiral Arms of a Triple Protostar System Imaged in Molecular Lines
Published 2023-01-01“…Most stars form in multiple-star systems. For a better understanding of their formation processes, it is important to resolve the individual protostellar components and the surrounding envelope and disk material at the earliest possible formation epoch, because the formation history can be lost in a few orbital timescales. …”
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On Encounter Rates in Star Clusters
Published 2023-01-01“…Close encounters between stars in star-forming regions are important as they can perturb or destroy protoplanetary disks, young planetary systems, and multiple-star systems. We simulate simple, virialized, equal-mass N -body star clusters and find that both the rate and the total number of encounters between stars vary by factors of several in statistically identical clusters due to the stochastic/chaotic details of the orbits and stellar dynamics. …”
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ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): A Forming Quadruple System with Continuum “Ribbons” and Intricate Outflows
Published 2023-01-01“…One of the most poorly understood aspects of low-mass star formation is how multiple-star systems are formed. Here we present the results of Atacama Large Millimeter/submillimeter Array (ALMA) Band 6 observations toward a forming quadruple protostellar system, G206.93-16.61E2, in the Orion B molecular cloud. …”
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SCATTER: A New Common Envelope Formalism
Published 2023-01-01“…Here we focus on CEs in binaries, and the follow-up paper extends our formalism to multiple-star systems within which a CE occurs.…”
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Improving CMD Areal Density Analysis: Algorithms and Strategies
Published 2014-06-01“…Observational errors and multiple star systems, along with various single star characteristics and phenomena, are modeled directly via the Functional Statistics Algorithm (FSA). …”
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TIC 168789840: A Sextuply Eclipsing Sextuple Star System
Published 2021“…As a consequence of its rare composition, structure, and orientation, this object can provide important new insight into the formation, dynamics, and evolution of multiple star systems. Future observations could reveal if the intermediate and outer orbital planes are all aligned with the planes of the three inner eclipsing binaries.…”
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On the nature and evolution of the unique binary pulsar J1903+0327
Published 2010“…(abridged) PSR J1903+0327, a millisecond pulsar in an eccentric (e = 0.44) 95-day orbit with a (~ 1Msun) companion poses a challenge to our understanding of stellar evolution in binary and multiple-star systems. Here we describe optical and radio observations which rule out most of the scenarios proposed to explain formation of this system. …”
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Triple Evolution: An Important Channel in the Formation of Type Ia Supernovae
Published 2023-01-01“…Since the predicted SN Ia rates from WDs in binaries are thought to be insufficient to explain the observed SN Ia rate, it is important to study similar interactions in higher-order multiple-star systems such as triple systems. We use the evolutionary population synthesis code Multiple Stellar Evolution (MSE) to study the stellar evolution, binary interactions, and gravitational dynamics of the triple-star systems. …”
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TIC 168789840: A Sextuply Eclipsing Sextuple Star System
Published 2022“…As a consequence of its rare composition, structure, and orientation, this object can provide important new insight into the formation, dynamics, and evolution of multiple star systems. Future observations could reveal if the intermediate and outer orbital planes are all aligned with the planes of the three inner eclipsing binaries.…”
Get full text
Article