ParaStell: parametric modeling and neutronics support for stellarator fusion power plants by Connor Moreno, Aaron Bader, Aaron Bader, Paul Wilson

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Considerations on Stellarator’s Optimization from the Perspective of the Energy Confinement Time Scaling Laws by Andrea Murari, Emmanuele Peluso, Luca Spolladore, Jesus Vega, Michela Gelfusa

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Cambridge workshop on cool stars, stellar systems, and the sun : [Proceedings]/ by Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (2nd : 1981 : Cambridge), Giampapa, M. S., Golub, L.

Suppression of pfirsch-schluter current by vertical magnetic field in stellarators / by 243354 Pustovitov, V. D.

Subjects: “…Stellarators…”

Stellar interiors [compact disc] : physical principles, structure, and evolution / by 212389 Hansen, Carl J., Kawaler, Steven D., Trimble, Virginia

Storytelling with you : plan, create, and deliver a stellar presentation / by Knaflic, Cole Nussbaumer, author

Solar, stellar and galactic connections between particle physics and astrophysics / by Carraminana, Alberto, Guzman, Francisco Siddhartha, Matos, Tonatiuh

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Anisotropic compact stellar objects with a slow rotation effect by Lipi Baskey, Shyam Das, Farook Rahaman

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Clustering Properties of Intermediate and High-mass Young Stellar Objects by Miguel Vioque, Manuel Cavieres, Michelangelo Pantaleoni González, Álvaro Ribas, René D. Oudmaijer, Ignacio Mendigutía, Lena Kilian, Héctor Cánovas, Michael A. Kuhn

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Coarse-grained gyrokinetics for the critical ion temperature gradient in stellarators by G. T. Roberg-Clark, G. G. Plunk, P. Xanthopoulos

“…Thanks to its simplicity, this novel formalism yields an estimate for the critical gradient with a computational cost low enough for application to stellarator optimization. When comparing against a gyrokinetic solver, our results show good agreement for an assortment of stellarator designs. …”
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Detecting Isolated Stellar-mass Black Holes with the Roman Telescope by Sedighe Sajadian, Kailash C. Sahu

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The Mass Accretion Rate and Stellar Properties in Class I Protostars by Eleonora Fiorellino, Łukasz Tychoniec, Fernando Cruz-Sáenz de Miera, Simone Antoniucci, Ágnes Kóspál, Carlo F. Manara, Brunella Nisini, Giovanni Rosotti

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In the Trenches of the Solar–Stellar Connection. VII. Wilson–Bappu 2022 by Thomas Ayres

Subjects: “…Stellar spectral lines…”
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Large dynamic range stellar radiation simulation optical system by Yu Zhang, Yuegang Fu, Qiang Liu, Li Wang, Songzhou Yang, Shitong Liang, Jian Zhang, Jun Zhong, Bin Zhao, Yao Meng

“…Abstract For the current stellar spectral simulation can not realize the stellar color temperature information with large dynamic range simulation, this paper proposes a broad spectrum high-resolution subdivision and spatial beam zoning modulation combined with a large dynamic range of stellar radiation information simulation method, designed a kind of imaging and non-imaging stellar radiation information simulation optical system, using an optical system to achieve multi-color temperature spectrum and large dynamic range stellar simulation. …”
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The Major Role of Eccentricity in the Evolution of Colliding Pulsar-Stellar Winds by Maxim V. Barkov, Valenti Bosch-Ramon

“…The relativistic pulsar wind and the non-relativistic stellar outflows interact along the orbit, producing ultrarelativistic particles that radiate from radio to gamma rays. …”
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A Hierarchical Bayesian Framework for Inferring the Stellar Obliquity Distribution by Jiayin Dong, Daniel Foreman-Mackey

“…In transiting-exoplanet observations, only the sky-projected stellar obliquity can be measured, but this can be deprojected using an estimate of the stellar obliquity. …”
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Stellar s-process neutron capture cross sections on ASe and ACe by Sahoo Rudra N., Tessler Moshe, Halfon Shlomi, Kijel Dani, Kreisel Arik, Paul Michael, Shor Asher, Weissman Leo

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Latitudinal Propagation of Thermal Rossby Waves in Stellar Convection Zones by Rekha Jain, Bradley W. Hindman

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A New Stellar Mass Proxy for Subhalo Abundance Matching by Chen-Yu Chuang, Yen-Ting Lin

“…In essence, the SHAM framework is to find a dark matter halo property that best correlates with an attribute of galaxies, such as stellar mass. The peak value of the maximum circular velocity ( ${V}_{\max }$ ) a halo/subhalo has ever attained throughout its lifetime, V _peak , has been a popular choice for SHAM. …”
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Atmospheric and Fundamental Parameters of the Individual Components of Multiple Stellar Systems by Enas M. Abu-Alrob, Abdallah M. Hussein, Mashhoor A. Al-Wardat

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