Self-similar shocks in polytropic gas flows around star-forming regions [PDF]
Yuqing Lou, Yang Gao
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Protocol for forming G-quadruplexes from double-stranded DNA during transcription. [PDF]
Zhang J, Gong J, Chen J, Chen H.
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Escape of Ionizing Radiation from Star-forming Regions in Young Galaxies [PDF]
Alexei O. Razoumov+1 more
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[Ar III]/[O III] and [S III]/[O III]: well-behaved oxygen abundance indicators for HII regions and star forming galaxies [PDF]
G. Stasińska
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Hierarchically Structured and Tunable Hydrogel Patches: Design, Characterization, and Application. [PDF]
Steinbeck L+7 more
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Full‐Polarization Observations of OH Masers in Massive Star‐forming Regions. II. Maser Properties and the Interpretation of Polarization [PDF]
Vincent L. Fish, M. J. Reid
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Polar vortex hidden in twisted bilayers of paraelectric SrTiO3. [PDF]
Sha H+8 more
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A Comparative Study of Two Synthesis Methods for Poly(Acrylic Acid-<i>Co</i>-Acrylamide) Incorporating a Hyperbranched Star-Shaped Monomer. [PDF]
Brito RSM+7 more
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Efficient Cow Body Condition Scoring Using BCS-YOLO: A Lightweight, Knowledge Distillation-Based Method. [PDF]
Zheng Z, Wang Z, Weng Z.
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Collapse scenarios in magnetized star-forming regions
[spa] La turbulencia, el campo magnético y la gravedad juegan un papel importante en la formación estelar. Aunque se ha mostrado que el campo magnético es importante, sólo se han llevado a cabo un número limitado de trabajos combinando el estudio del campo magnético y la cinemática del gas. Este tipo de trabajos son esenciales para estudiar la gravedad
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