dynamical modeling
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2022 ◽  
Vol 163 (2) ◽  
pp. 49
Author(s):  
N. Luber ◽  
Sarah Pearson ◽  
Mary E. Putman ◽  
Gurtina Besla ◽  
Sabrina Stierwalt ◽  
...  

Abstract We present resolved H i synthesis maps from the Very Large Array of three interacting dwarf systems: the NGC 3664 dwarf pair, the NGC 3264 dwarf pair, and the UGC 4638 dwarf triplet. All three dwarf systems are captured at various stages of interaction and span a range of environments. We detect clear hallmarks of tidal interactions through the presence of H i bridges and diffuse H i extensions that surround the dwarfs. We overlay the H i data on Pan-STARRS r-band images and find further evidence of tidal interactions through coincident distorted H i and tidal stellar features in NGC 3264 and UGC 4638, and an unwound spiral arm pointing toward its smaller companion in NGC 3264. In UGC 4638, both the gas and diffuse stars are extended to similar radii east of the primary, which could indicate that the smaller dwarf in the system has already completed one pass through the primary. We additionally find that our three systems, and those from the Local Volume TiNy Titans survey, are not H i deficient and thus the interaction has not resulted in a loss of gas from the systems. A comparison with noninteracting dwarf galaxies shows that the interactions have a significant impact on the kinematics of the systems. Our new resolved H i kinematics, combined with detailed stellar and H i morphologies, provide crucial constraints for future dynamical modeling of hierarchical mergers and the baryon cycle at the low-mass scale.


2021 ◽  
pp. 183-202
Author(s):  
Muhammad Shahzad ◽  
Faisal Sultan ◽  
Mehboob Ali ◽  
Soma Mustafa
Keyword(s):  

2021 ◽  
pp. 503-516
Author(s):  
Olukayode Adebimpe ◽  
Olukayode Adeyemo ◽  
Nathaniel Oladejo ◽  
Olajumoke Oludoun ◽  
Oluwakemi Abiodun ◽  
...  

Author(s):  
Juan Li ◽  
Zhen Jin ◽  
Youming Wang ◽  
Xiangdong Sun ◽  
Quangang Xu ◽  
...  

2021 ◽  
pp. 167-192
Author(s):  
Marek Pokropski
Keyword(s):  

Author(s):  
Sarah F Ackley ◽  
Justin Lessler ◽  
M Maria Glymour

Abstract Dynamical models, commonly used in infectious disease epidemiology, are formal mathematical representations of time-changing systems or processes. For many chronic disease epidemiologists, the link between dynamical models and predominant causal inference paradigms is unclear. This commentary explains the use of dynamical models for representing causal systems and the relevance of dynamical models for causal inference. In certain simple settings, dynamical modeling and conventional statistical methods (e.g., regression-based methods) are equivalent, but dynamical modeling has advantages over conventional statistical methods for many causal inference problems. Dynamical models can be used to transparently encode complex biological knowledge, interference and spillover, effect modification, and variables that influence each other in continuous time. As our knowledge of biological and social systems and access to computational resources increases, there will be a growing utility for a variety of mathematical modeling tools in epidemiology.


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