solar-and-stellar-astrophysics

Documents about solar-and-stellar-astrophysics

• The POKEMON Speckle Survey of Nearby M Dwarfs. III. The Stellar Multiplicity Rate of M Dwarfs within 15 pc#131208arXiv (OAI)
• Can COSI detect $γ$-ray lines from rare isotopes produced in the astrophysical intermediate neutron-capture process?#608888arXiv (OAI Expanded)
• YSO peculiar motions and magnetic fields Do young stars retain their natal magnetic field orientation?#608911arXiv (OAI Expanded)
• Kratos-linerad: GPU-accelerated Monte Carlo radiative transfer of lines with efficient imaging#608973arXiv (OAI Expanded)
• JWST/NIRSpec Spectra for Three Ultracool Brown Dwarfs Detected in Extragalactic Surveys: Further Evidence for Phosphine Absorption#609211arXiv (OAI Expanded)
• Local Interstellar Flow Parameters from the First Intersection of IMAP-Lo's Parameter Tubes#609353arXiv (OAI Expanded)
• Modeling the Dynamics and Thermochemistry for the Outer Atmospheres of the Ultra-hot Jupiter WASP-121b#609867arXiv (All)
• Can COSI detect $γ$-ray lines from rare isotopes produced in the astrophysical intermediate neutron-capture process?#609950arXiv (All)
• YSO peculiar motions and magnetic fields Do young stars retain their natal magnetic field orientation?#609973arXiv (All)
• Kratos-linerad: GPU-accelerated Monte Carlo radiative transfer of lines with efficient imaging#610035arXiv (All)
• Detection of Aliphatically Deuterated Aromatic Hydrocarbons in the Large Magellanic Cloud 30 Doradus Star-Forming Complex#610943arXiv (OAI Expanded)
• Detection of Aliphatically Deuterated Aromatic Hydrocarbons in the Large Magellanic Cloud 30 Doradus Star-Forming Complex#612420arXiv (All)
• Panchromatic JWST Observations and Models of the Dim Type Iax Supernova 2024vjm at 200 days#612471arXiv (All)
• A self-consistent solar coronal heating model by Alfvenic waves#612643arXiv (All)

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