[HTML][HTML] Final moments. II. Observational properties and physical modeling of circumstellar-material-interacting Type II supernovae

WV Jacobson-Galán, L Dessart… - The Astrophysical …, 2024 - new.iopscience.iop.org
We present ultraviolet/optical/near-infrared observations and modeling of Type II
supernovae (SNe II) whose early time (δt< 2 days) spectra show transient, narrow emission …

Ejecta, rings, and dust in SN 1987A with JWST MIRI/MRS

OC Jones, PJ Kavanagh, MJ Barlow… - The Astrophysical …, 2023 - iopscience.iop.org
Supernova (SN) 1987A is the nearest supernova in∼ 400 yr. Using the JWST MIRI Medium
Resolution Spectrograph, we spatially resolved the ejecta, equatorial ring (ER), and outer …

The formation and cosmic evolution of dust in the early Universe: I. Dust sources

R Schneider, R Maiolino - The Astronomy and Astrophysics Review, 2024 - Springer
Dust-obscured star formation has dominated the cosmic history of star formation, since z≃ 4.
However, the recent finding of significant amount of dust in galaxies out to z≃ 8 has opened …

Keck Infrared Transient Survey. I. Survey Description and Data Release 1

S Tinyanont, RJ Foley, K Taggart… - Publications of the …, 2024 - iopscience.iop.org
Abstract We present the Keck Infrared Transient Survey, a NASA Key Strategic Mission
Support program to obtain near-infrared (NIR) spectra of astrophysical transients of all types …

A Hubble Space Telescope Search for r-Process Nucleosynthesis in Gamma-ray Burst Supernovae

JC Rastinejad, W Fong, AJ Levan… - The Astrophysical …, 2024 - iopscience.iop.org
The existence of a secondary (in addition to compact object mergers) source of heavy
element (r-process) nucleosynthesis, the core-collapse of rapidly rotating and highly …

Carbonaceous dust grains seen in the first billion years of cosmic time

J Witstok, I Shivaei, R Smit, R Maiolino, S Carniani… - Nature, 2023 - nature.com
Large dust reservoirs (up to approximately 108 M⊙) have been detected,–in galaxies out to
redshift z≃ 8, when the age of the Universe was only about 600 Myr. Generating substantial …

Shockingly bright warm carbon monoxide molecular features in the supernova remnant Cassiopeia A revealed by JWST

J Rho, SH Park, R Arendt, M Matsuura… - The Astrophysical …, 2024 - iopscience.iop.org
Abstract We present JWST NIRCam (F356W and F444W filters) and MIRI (F770W) images
and NIRSpec Integral Field Unit (IFU) spectroscopy of the young Galactic supernova …

Serendipitous detection of the dusty Type IIL SN 1980K with JWST/MIRI

S Zsíros, T Szalai, I De Looze, A Sarangi… - Monthly Notices of …, 2024 - academic.oup.com
We present mid-infrared (mid-IR) imaging of the Type IIL supernova (SN) 1980K with the
JWST more than 40 yr post-explosion. SN 1980K, located in the nearby (D≈ 7 Mpc)'SN …

Supernovae in 2023 (review): breakthroughs by late observations

N Soker - arXiv preprint arXiv:2311.17732, 2023 - arxiv.org
I present a review of how late observations of supernovae, of the nebular phase, and much
later of supernova remnants (SNRs), and their analysis in 2023 made progress towards …

[HTML][HTML] Supernova Ejecta with Crystalline Silicate Dust in the Supernova Remnant MSH 15–52

HJ Kim, BC Koo, T Onaka - The Astrophysical Journal, 2024 - new.iopscience.iop.org
IRAS 15099-5856 in the young supernova remnant (SNR) MSH 15− 52 is the first and only
SNR-associated object with crystalline silicate dust detected so far, although its nature and …