Results 111 to 120 of about 372,210 (210)

87th Annual Meeting of the Meteoritical Society 2025: Cover

open access: yes
Meteoritics &Planetary Science, Volume 60, Issue S1, August 2025.
wiley   +1 more source

The End of the Road for Far-infrared Reddening Maps? Evidence for Reddening Errors Driven by Changes in Polycyclic Aromatic Hydrocarbon Abundance

open access: yesThe Astrophysical Journal
Accurate correction for extinction by Galactic dust is essential for studying the extragalactic sky. In the low-extinction regions of the Ursa Major molecular cloud complex, we demonstrate that Galactic dust reddening maps constructed from observations ...
Dennis Lee   +3 more
doaj   +1 more source

An Empirical Extinction Curve Revealed by Gaia XP Spectra and LAMOST

open access: yesThe Astrophysical Journal
We present a direct measurement of extinction curves using corrected Gaia XP spectra of the common sources in Gaia DR3 and LAMOST DR7. Our analysis of approximately 370,000 high-quality samples yielded a high-precision average extinction curve for the ...
Ruoyi Zhang   +6 more
doaj   +1 more source

Astro 2020: Astromineralogy of interstellar dust with X-ray spectroscopy [PDF]

open access: green, 2019
Lía Corrales   +18 more
openalex   +1 more source

The Spheroidal Analog Method for Modeling Irregular Porous Aggregates

open access: yesThe Astrophysical Journal
It is shown that the optical properties of an irregular porous grain with effective radius a _eff  ≲ 3 λ (where λ is the wavelength) can be well approximated by a “spheroidal analog”: a spheroid with appropriate axial ratio and size, with a dielectric ...
B. T. Draine
doaj   +1 more source

Modeling Dust Production, Growth, and Destruction in Reionization-era Galaxies with the CROC Simulations. II. Predicting the Dust Content of High-redshift Galaxies

open access: yesThe Astrophysical Journal
We model the interstellar dust content of the reionization era with a suite of cosmological, fluid-dynamical simulations of galaxies with stellar masses ranging from ∼10 ^5 to 10 ^9 M _⊙ in the first 1.2 Gyr of the Universe.
Clarke J. Esmerian, Nickolay Y. Gnedin
doaj   +1 more source

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