Results 71 to 80 of about 5,625,011 (180)
Gas and dust in a submillimeter galaxy at ⱬ = 4.24 from the herschel atlas [PDF]
We report ground-based follow-up observations of the exceptional source, ID 141, one of the brightest sources detected so far in the Herschel Astrophysical Terahertz Large Area Survey cosmological survey. ID 141 was observed using the IRAM 30 m telescope
Itziar Aretxaga, David Hughes
core
The Formation of Astrophysical Dust
The formation of carbonaceous and silicate precursor molecules to astrophysical dust grains is investigated. Using density functional theory (DFT) in combination with global optimization techniques, the ground-state binding energies of dust precursors ...
Mauney, Christopher M.
core +4 more sources
Modeling the Redistribution of Dust Across the Martian Surface for Mars Years 24 to 36
Abstract Global Dust Events (GDEs) transport huge amounts of dust across the Martian atmosphere. GDEs occur only every few Mars Years (MYs), but the reasons behind this inter‐annual variability remain poorly understood. The question whether surface dust exhaustion and subsequent replenishment explain this variability remains open.
Demetrius Ramette +3 more
wiley +1 more source
Mechanical properties of small bodies such as dust, pebbles, and planetesimals are key to better understanding the formation of planetary systems against their collisional destruction.
Hiroshi Kimura +17 more
doaj +1 more source
Modeling Dust in the Interstellar Medium
We are in a very special moment for the study of the interstellar medium (ISM). The Spitzer Space Telescope had provided, and currently Herschel Space Observatory is providing, invaluable infrared (IR) observations of a variety of astrophysical ...
Aniano Porcile, Gonzalo Jorge
core
Radiative Processes in Astrophysical and Laboratory Plasmas
Radiative processes are among the most fundamental ones in plasma physics. In general, they can be quite complicated and require a full kinetic description.
Munirov, Vadim R.
core
The tensile strength of solid particles is the key parameter that controls not only the formation of planetesimals in protoplanetary disks but also outburst and splitting of comets and rotational bursting of asteroids in planetary systems.
Hiroshi Kimura +18 more
doaj +1 more source
Geochemistry and risk assessment of street dust in Luanda, Angola, a tropical urban environment [PDF]
A total of 92 samples of street dust were collected in Luanda, Angola, were sieved below 100 μm, and analysed by ICP-MS for 35 elements after an aqua-regia digestion.
Miguel García, Eduardo de +1 more
core +1 more source
Probing the Subparsec Dust of a Supermassive Black Hole with the Tidal Disruption Event AT 2020mot
AT 2020mot is a typical UV/optical tidal disruption event (TDE) with no radio or X-ray signatures in a quiescent host. We find an i -band excess and rebrightening along the decline of the light curve which could be due to two consecutive dust echoes from
Megan Newsome +12 more
doaj +1 more source
Dust Growth in ALMA Rings. II. Dusty Rossby Wave Instability
Annular substructures serve as ideal venues for planetesimal formation. In this series, we investigate the linear stage of dust growth within rings. The first paper in this series examines the global streaming instability, while this study focuses on the
Can Cui +7 more
doaj +1 more source

