Results 111 to 120 of about 372,210 (210)
87th Annual Meeting of the Meteoritical Society 2025: Cover
Meteoritics &Planetary Science, Volume 60, Issue S1, August 2025.
wiley +1 more source
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
Interstellar Dust—Reply to Duley's Criticisms [PDF]
N. C. Wickramasinghe, K. Nandy
openalex +1 more source
A Comprehensive Model of Morphologically Realistic Cosmic Dust Particles: An Application to Mimic the Unusual Polarization Properties of the Interstellar Comet 2I/Borisov [PDF]
Prithish Halder, Sujan Sengupta
openalex +1 more source
An Empirical Extinction Curve Revealed by Gaia XP Spectra and LAMOST
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]
Lía Corrales +18 more
openalex +1 more source
On interstellar light polarization by diamagnetic silicate and carbon dust in the infrared [PDF]
R. Papoular
openalex +1 more source
The Spheroidal Analog Method for Modeling Irregular Porous Aggregates
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
Dust emission in the diffuse interstellar medium from far-infrared to millimeter: new constraints from WMAP [PDF]
G. Lagache
openalex +1 more source
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

