... Dust evolution across the CO snowline in a protoplanetary disk . Dust grains from the heart of supernovae . ... Dust evolution across the CO snowline in a protoplanetary disk . Dust grains from the heart of supernovae . ...
... of quantities (Hubble type, inclination, dust optical thickness, dust distribution and extinction properties) for a large wavelength interval, ranging from 1250A to the K band, thus finally providing a comprehensive atlas of dust extinction in galaxies ...
... An ESF exploratory workshop on: . Tracing Dust in Spiral Galaxies: .. ... next few years, several observing facilities will allow to study the dust content of spiral galaxies with unprecedented detail ...
... of dust grains mainly due to collisions between energetic gas particles and dust ... dust yield that they have obtained leads to a SN dust production rate almost an ...
... An ESF exploratory workshop on: . Tracing Dust in Spiral Galaxies: .. ... Institut d'Astrophysique Spatiale, Universite Paris-Sud . Dust in different Milky Way environments . Buat Veronique . ...
... Dust lying in the spiral arms of the foreground galaxy stands out where it absorbs light from the more distant galaxy. ... This silhouetting shows us where the interstellar dust clouds are located, and how much light they absorb. ...
... Dust and Gas Surrounding Star R Coronae Australis . Credit: F. Comeron , WFI , MPG , La Silla Observatory , ESO . ... The dust is so thick on the upper left of the above photograph that little light from background stars comes through. ...