Results 101 to 110 of about 25,802 (223)

Imaging the circumstellar dust around AGB stars with PolCor [PDF]

open access: bronze, 2011
S. Ramstedt   +4 more
openalex   +1 more source

Extraordinary Late-Time Infrared Emission of Type IIn Supernovae

open access: yes, 2002
Near-Infrared (NIR) observations are presented for five Type IIn supernovae (SN 1995N, SN 1997ab, SN 1998S, SN 1999Z, and SN 1999el) that exhibit strong infrared excesses at late times (t >= 100 d).
Baird M. D.   +27 more
core   +1 more source

Long-period Variable Stars in NGC 147 and NGC 185. II. Their Dust Production

open access: yesThe Astrophysical Journal
This study presents a comparative analysis of mass-loss and dust production rates in the dwarf galaxies NGC 147 and NGC 185, focusing on long-period variables (LPVs) and pulsating asymptotic giant branch stars as primary indicators of dust feedback into ...
Hamidreza Mahani   +8 more
doaj   +1 more source

Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling

open access: yesThe Astrophysical Journal
The evolution of dust in core-collapse supernovae (SNe), in general, is poorly constrained owing to a lack of infrared observations a few years after explosion. Most theories of dust formation in SNe heavily rely only on SN 1987A.
Arkaprabha Sarangi   +22 more
doaj   +1 more source

Dust dynamics in planet-forming discs in binary systems. [PDF]

open access: yesEur Phys J Plus, 2023
Zagaria F   +3 more
europepmc   +1 more source

Discovery of stars surrounded by iron dust in the LMC

open access: yes, 2019
We consider a small sample of oxygen-rich, asymptotic giant branch stars in the Large Magellanic Cloud, observed by the Spitzer Space Telescope, exhibiting a peculiar spectral energy distribution, which can be hardly explained by the common assumption ...
Dell'Agli, F.   +6 more
core   +1 more source

The Near-infrared Echo from SN 2023xgo: Evidence for a Massive Presupernova Eruption in a Type Ibn/Icn Supernova

open access: yesThe Astrophysical Journal Letters
We present near-infrared (NIR) and optical observations and analysis of the Type Ibn/Icn supernova (SN) 2023xgo, spanning the period from 2 to 100 days past explosion.
Masayuki Yamanaka, Takahiro Nagayama
doaj   +1 more source

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