Results 131 to 140 of about 2,475,925 (212)
Current explanations of the mass-loss mechanism for stripped-envelope supernovae (SNe) remain divided between single and binary progenitor systems. Here we obtain deep ultraviolet (UV) imaging with the Hubble Space Telescope (HST) of the Type Ic SN ...
Benjamin F. Williams +21 more
doaj +1 more source
Enabling Early Transient Discovery in LSST via Difference Imaging with DECam
We present SLIDE , a pipeline that enables transient discovery in data from the Vera C. Rubin Observatory’s Legacy Survey of Space and Time (LSST), using archival images from the Dark Energy Camera as templates for difference imaging.
Yize Dong +60 more
doaj +1 more source
SN 2023taz: Implications for the UV Diversity of Superluminous Supernovae
Superluminous supernovae (SLSNe) are some of the brightest explosions in the Universe, representing the extremes of stellar deaths. At the upper end of their distribution is SN 2023taz, in a dwarf galaxy at z = 0.407.
Aysha Aamer +24 more
doaj +1 more source
Understanding the Neutrino Dynamics in Pre-Core Collapse Supernovae [PDF]
Core-collapse supernovae represent some of the most energetic events in the universe, where neutrino interactions play a crucial role in the explosion mechanism.
Bhat, Yash
core +1 more source
SN 2017hcc and SN 2023usc—A Comparative Spectroscopic Study of Type IIn Supernovae
We report on a spectroscopic study of the bright, nearby type IIn supernovae SN 2017hcc and SN 2023usc using data obtained from the Himalayan Chandra Telescope.
V. Sethulakshmi +3 more
doaj +1 more source
Analysis of a Type II Supernova Candidate at z = 3.19 from JWST’s COSMOS-Web Survey
The launch of the James Webb Space Telescope (JWST) has enabled the discovery of a small but increasing sample of high-redshift core-collapse supernovae (CC SNe), which provide new tests of massive star evolution in the early Universe.
Valeria Aparicio +23 more
doaj +1 more source
SN 2019cqc: A Hydrogen-rich Superluminous Supernova Showing Electron-scattering Signatures
Hydrogen-rich superluminous supernovae without narrow emission lines (SLSNe-II) are rare transients whose powering mechanisms remain debated, particularly the role of circumstellar medium (CSM) interaction.
Dinesh Hebbar +17 more
doaj +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Contents
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 2-29, August 2025.
wiley +1 more source

