SN 2023fyq is the first Type Ibn supernova with a directly detected hot luminous progenitor consistent with a low-mass helium star in a binary system, based on pre-explosion imaging, disappearance confirmation, and multi-wavelength environmental analysis.
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Introduces a LIV term δ_LIV (p·n)^2 in the Z boson dispersion relation and outlines a search strategy in Drell-Yan processes at |Y|>4 for sensitivity down to |δ_LIV|~10^{-8} with possible sidereal modulations.
New photometry of RZ LMi and KV Dra detects superhumps during superoutbursts, determines periods and amplitudes, clarifies ER UMa and WZ Sge subclassifications, and measures a 0.0586-day orbital period for KV Dra.
A review of interstellar dust production, destruction, accretion, and depletion that concludes dust growth in cold clouds is critical and high-redshift dust budgets remain poorly constrained.
citing papers explorer
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SN 2023fyq: direct detection of a Type Ibn supernova progenitor and its multi-wavelength environmental constraints
SN 2023fyq is the first Type Ibn supernova with a directly detected hot luminous progenitor consistent with a low-mass helium star in a binary system, based on pre-explosion imaging, disappearance confirmation, and multi-wavelength environmental analysis.
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Probing Lorentz Invariance Violation in Z Boson Mass Measurements at High-Energy Colliders
Introduces a LIV term δ_LIV (p·n)^2 in the Z boson dispersion relation and outlines a search strategy in Drell-Yan processes at |Y|>4 for sensitivity down to |δ_LIV|~10^{-8} with possible sidereal modulations.
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Photometric light curves analysis of SU UMa-type dwarf novae: the case of RZ LMi and KV Dra
New photometry of RZ LMi and KV Dra detects superhumps during superoutbursts, determines periods and amplitudes, clarifies ER UMa and WZ Sge subclassifications, and measures a 0.0586-day orbital period for KV Dra.
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Interstellar dust production, destruction and effects of dust depletion in galaxies
A review of interstellar dust production, destruction, accretion, and depletion that concludes dust growth in cold clouds is critical and high-redshift dust budgets remain poorly constrained.