Results 101 to 110 of about 2,154,904 (218)
The circumstellar matter of supernova 2014J and the core-degenerate scenario [PDF]
Accepted to ...
openaire +2 more sources
SN 2024dy: Dust Formation in a Long-lived Type IIn Supernova and Constraints on the Dust Mass
Type IIn supernovae (SNe) are a subclass of core-collapse SNe powered by interaction between the ejecta and the dense circumstellar material. Among them, long-lived Type IIn events are characterized by luminous, long-duration light curves with high ...
Sota Goto +12 more
doaj +1 more source
SN 2021ukt: A Transitional Supernova with a Short Plateau and Persistent Interaction
We present spectroscopic and photometric observations of SN 2021ukt, a peculiar short-plateau object that was originally identified as a Type IIn supernovae (SN) and later underwent an unprecedented transition to a Type Ib (possibly Type IIb) SN.
Neil R. Pichay +23 more
doaj +1 more source
Observational constraints on circumstellar dust [PDF]
There is an enormous range in the properties of stars that are losing mass. The red giants responsible for injecting roughly half or more of the material into the interstellar medium are reviewed. The physical properties are described for the out flowing
Jura, M.
core
The excitation of circumstellar C
Context. Observations of the circumstellar envelopes of post-asymptotic giant branch (post-AGB) stars provide information about their mass-loss history during the AGB phase and about the chemistry inside envelopes after that phase. Aims.
M. Pułecka +3 more
core +1 more source
Transients by Black Hole Formation from Red Supergiants: Impact of Dense Circumstellar Matter [PDF]
Failed supernovae (SNe), which are likely the main channel for forming stellar-mass black holes, are predicted to accompany mass ejections much weaker than typical core-collapse SNe.
Piro, Anthony L. +3 more
core +1 more source
SN 2022erq: A Superluminous Thermonuclear Supernova with Escalating Preexplosion Mass Loss
We present a photometric and spectroscopic study of the superluminous Type Ia supernova SN 2022erq. Its early spectra, dominated by iron-group elements with weak intermediate-mass features, might indicate highly efficient nuclear burning, broadly similar
Qian Zhai +53 more
doaj +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
Circumstellar interaction of supernova (SN) ejecta is an essential process in its evolution, and observations of SNe have found the signature of circumstellar interaction in both the early and late evolutionary phases of SNe. In this Letter, we show that
Tomoki Matsuoka +2 more
doaj +1 more source
Scattered light imaging of protoplanetary disks provides key insights on the geometry and dust properties in the disk surface. Here, we present James Webb Space Telescope (JWST) 2–21 μ m images of a 1000 au radius edge-on protoplanetary disk surrounding ...
Gaspard Duchêne +8 more
doaj +1 more source

