3D SPH simulations show that localized, mildly super-Keplerian equatorial mass ejections with high viscosity reproduce the photometric, spectroscopic, and polarimetric signatures of Be star flicker events.
M., Baliber, N., Bianco, F
3 Pith papers cite this work. Polarity classification is still indexing.
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XRF 241001A, a soft faint burst at z=0.573 detected by SVOM, hosted a broad-line Type Ic supernova (SN 2024aiiq), indicating a collapsar with a weak on-axis jet.
Three new warm Jupiters (periods 11.3–44.4 days, masses 0.51–1.29 M_J, radii ~0.97–0.98 R_J) were confirmed via TESS photometry and follow-up radial velocities and light curves.
citing papers explorer
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The birth of Be star disks III. SPH models of localised mass ejections
3D SPH simulations show that localized, mildly super-Keplerian equatorial mass ejections with high viscosity reproduce the photometric, spectroscopic, and polarimetric signatures of Be star flicker events.
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XRF 241001A/SN 2024aiiq: A faint soft X-ray transient detected by SVOM with a broad-line type Ic supernova revealed by JWST
XRF 241001A, a soft faint burst at z=0.573 detected by SVOM, hosted a broad-line Type Ic supernova (SN 2024aiiq), indicating a collapsar with a weak on-axis jet.
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PLATOSpec's first results: Three new transiting warm Jupiters from the WINE survey TIC 147027702, TIC 245076932 and TIC 87422071
Three new warm Jupiters (periods 11.3–44.4 days, masses 0.51–1.29 M_J, radii ~0.97–0.98 R_J) were confirmed via TESS photometry and follow-up radial velocities and light curves.