Results 81 to 90 of about 584 (186)
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
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The mystery of unidentified infrared emission bands. [PDF]
Kwok S.
europepmc +1 more source
A Spectroscopic and Photometric Study of MWC 342 and Its B[e] Phenomenon over the Last 40 Years
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
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Transients by Black Hole Formation from Red Supergiants: Impact of Dense Circumstellar Matter
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
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Radiation-driven acceleration in the expanding WR140 dust shell. [PDF]
Han Y, Tuthill PG, Lau RM, Soulain A.
europepmc +1 more source
86th Annual Meeting of the Meteoritical Society (2024)
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
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
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Hidden metallic iron in amorphous silicate dust?
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
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A Shock Crashing into Confined Dense Circumstellar Matter Brightens the Nascent SN 2023ixf
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
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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
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