Results 81 to 90 of about 584 (186)

Evidence for an Instability-induced Binary Merger in the Double-peaked, Helium-rich Type IIn Supernova 2023zkd

open access: yesThe Astrophysical Journal
We present ultraviolet to infrared observations of the extraordinary Type IIn supernova 2023zkd (SN 2023zkd). Photometrically, it exhibits persistent and luminous precursor emission spanning ∼4 yr preceding discovery ( M _r  ≈ −15 mag, 1500 days in the ...
A. Gagliano   +45 more
doaj   +1 more source

A Spectroscopic and Photometric Study of MWC 342 and Its B[e] Phenomenon over the Last 40 Years

open access: yesGalaxies
MWC 342 (V1972 Cyg) was discovered nearly 90 years ago as an early-type emission-line star. It was among the first hot stars whose strong infrared excess was detected in the early 1970s.
Aigerim Zh. Akniyazova   +13 more
doaj   +1 more source

Transients by Black Hole Formation from Red Supergiants: Impact of Dense Circumstellar Matter

open access: yesThe Astrophysical Journal
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.
Daichi Tsuna   +3 more
doaj   +1 more source

Radiation-driven acceleration in the expanding WR140 dust shell. [PDF]

open access: yesNature, 2022
Han Y, Tuthill PG, Lau RM, Soulain A.
europepmc   +1 more source

86th Annual Meeting of the Meteoritical Society (2024)

open access: yes
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley   +1 more source

X-Ray Diagnostics of Cassiopeia A’s “Green Monster”: Evidence for Dense Shocked Circumstellar Plasma

open access: yesThe Astrophysical Journal Letters
The recent survey of the core-collapse supernova remnant Cassiopeia A (Cas A) with the MIRI instrument on board the James Webb Space Telescope (JWST) revealed a large structure in the interior region, referred to as the “Green Monster.” Although its ...
Jacco Vink   +6 more
doaj   +1 more source

Hidden metallic iron in amorphous silicate dust?

open access: yesAstronomy & Astrophysics
Context. Amorphous silicate dust is a major component in the interstellar and circumstellar dust formed in the outflow of asymptotic giant branch (AGB) stars.
Enomoto H.   +3 more
doaj   +1 more source

A Shock Crashing into Confined Dense Circumstellar Matter Brightens the Nascent SN 2023ixf

open access: yesThe Astrophysical Journal
Red supergiants may experience a short-lived period of episodic mass loss rather than steady winds before their core collapses, leading to dense circumstellar matter (CSM) close to core-collapse supernovae (SNe). Interaction of SN ejecta with such nearby
Maokai Hu, Lifan Wang, Xiaofeng Wang
doaj   +1 more source

exoALMA. XI. ALMA Observations and Hydrodynamic Models of LkCa 15: Implications for Planetary Mass Companions in the Dust Continuum Cavity

open access: yesThe Astrophysical Journal Letters
In the past decade, the Atacama Large Millimeter/submillimeter Array (ALMA) has revealed a plethora of substructures in the disks surrounding young stars.
Charles H. Gardner   +45 more
doaj   +1 more source

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