Results 31 to 40 of about 4,499,156 (300)
Characterizing the physical properties of dust grains in a protoplanetary disk is critical to comprehending the planet formation process. Our study presents Atacama Large Millimeter/submillimeter Array (ALMA) high-resolution observations of the young ...
Satoshi Ohashi +12 more
doaj +1 more source
Dust Formation in Hot Stellar Winds [PDF]
WC-type Wolf-Rayet stars show episodic or persistent infrared emission attributed to amorphous carbon grains forming in their winds. The process of dust formation in the hydrogen-poor environments characteristic of WC winds is reviewed and compared to the chemical pathway to soot particle production in AGB stars. Emphasis is put on the formation of the
I. Cherchneff, A.G.G.M. Tielens
openaire +1 more source
Indoor and outdoor dust in Damaturu Nigeria : composition, exposure and risk to human health [PDF]
Harmattan and Dust (sand) storms together with anthropogenic activities including the use of firewood and kerosene as fuel for cooking, and diesel/petrol generators for electricity generation are potential sources of particulate and gaseous pollutants in
Mohammed, Fatima Sule
core +4 more sources
The view that dust is essential to star formation is challenged on the ground that other interstellar constituents can provide more rapid cooling. From the evidence of stellar minimum masses it is suggested that self absorption of the radiation emitted by the coolant H2 is the dominant mechanism leading to the heating of a collapsing fragment.
openaire +1 more source
Dust mobilization and transport in the northern Sahara during SAMUM 2006 – a meteorological overview [PDF]
The SAMUM field campaign in southern Morocco in May/June 2006 provides valuable data to study the emission, and the horizontal and vertical transports of mineral dust in the Northern Sahara.
Wendisch, M. +33 more
core +1 more source
The Formation of Encke Meteoroids and Dust Trail [PDF]
manuscript in TeX, 10 figures (6 ps, 4 jpg); accepted by Icarus July 3 ...
Reach, William T. +3 more
openaire +2 more sources
Galaxy simulation with dust formation and destruction [PDF]
We perform smoothed particle hydrodynamics (SPH) simulations of an isolated galaxy with a new treatment for dust formation and destruction. To this aim, we treat dust and metal production self-consistently with star formation and supernova feedback. For dust, we consider a simplified model of grain size distribution by representing the entire range of ...
Aoyama, Shohei +6 more
openaire +2 more sources
Disk evolution, element abundances and cloud properties of young gas giant planets [PDF]
ChHc and PBR highlights financial support of the European Community under the FP7 program by an ERC starting grant. PW, IK, and WFT acknowledge funding from the European Union Seventh Framework Programme FP7-2011 under grant agreement No.
Kamp, I. +19 more
core +1 more source
Evading the dust fragmentation barrier with the streaming instability in protoplanetary disks
Context. The streaming instability (SI) is a leading candidate for reaching solid densities sufficient to trigger the gravitational collapse needed for the formation of planetesimals. However, dust growth barriers appear to impede the ability to assemble
Vallucci-Goy V. +3 more
doaj +1 more source
Dust formation and survival in supernova ejecta [PDF]
MNRAS ...
Bianchi, Simone, SCHNEIDER, Raffaella
openaire +2 more sources

