Dust emission from wet, low-emission coke quenching process
نویسندگان
چکیده
منابع مشابه
Dust emission from IRC + 10216
Infrared emission from the dust shell around IRC+10216 is analysed in detail, employing a self-consistent model for radiatively driven winds around late-type stars that couples the equations of motion and radiative transfer in the dust. The resulting model provides agreement with the wealth of available data, including the spectral energy distribution in the range 0.5–1000 μm, and visibility an...
متن کاملPolarized Microwave Emission from Dust
Polarized emission from dust is an important foreground that can hinder the progress in polarized CMB studies unless carefully accounted for. We discuss potential difficulties associated with the dust foreground, namely, the existence of different grain populations with very different emission/polarization properties and variations of the polarization yield with grain temperature. In this conte...
متن کاملPolarized Emission from Interstellar Dust
Observations of far-infrared (FIR) and submillimeter (SMM) polarized emission are used to study magnetic fields and dust grains in dense regions of the interstellar medium (ISM). These observations place constraints on models of molecular clouds, star-formation, grain alignment mechanisms, and grain size, shape, and composition. The FIR/SMM polarization is strongly dependent on wavelength. We h...
متن کاملDust Emission from Wet and Dry Playas in the Mojave Desert , USAt
Dust Emission from Wet and Dry Playas in the Mojave Desert, USAt Richard L. Reynolds,'* James c. Yount, I Marith Reheis, ' Harland Goldstein,1 Pat Chavez, Jr.? Robert Fulton,3 John Whitney, I Christopher Fuller and Richard M. Forester' , US. Geologicol Survey. Denver, Co. USA 2 US Geological Survey. Flagstaff. AZ, USA liB R A R Y 3 California Desert Studies Consortium. California State Universi...
متن کاملDust Emission from the Perseus Molecular Cloud
Using far-infrared emission maps taken by IRAS and Spitzer and a near-infrared extinction map derived from 2MASS data, we have made dust temperature and column density maps of the Perseus molecular cloud. We show that the emission from transiently heated very small grains (VSGs) and the big grain dust emissivity vary as a function of extinction and dust temperature, with higher dust emissivitie...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: E3S Web of Conferences
سال: 2018
ISSN: 2267-1242
DOI: 10.1051/e3sconf/20182801002