... Download: pdf . Session: Spitzer and dust surveys of the Magellanic System . Key Talk: Margaret Meixner . ... Millimetre dust emission as a tracer of molecular gas in galaxies: comparison of SMC and Local Giant Molecular Clouds . ...
... The dust grains in the disks have to grow from submicron to kilometre sizes within a few million years, and the largerst grains ... correlation with the 10-micron silicate dust feature, which probes the . inner disk. ...
... like red beads in a necklace) and the dust lanes lying along the arms and reaching ... Way we can recognise similar HII regions and dust lanes and we can then zoom in on ...
... Cores Astrochemistry OH Thermal Jets Masers Dust Continuum Cold Cores Outflows Class ... with MIR sources (24 m), all are associated with millimetre dust conFnuum emission ...
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Ссылки http://www.atnf.csiro.au/research/conferences/Parkes50th/SimonEllingsen.pdf -- 2473.2 Кб -- 08.11.2011 Похожие документы
... is emission from warm circumstellar dust; if so, the dust emissivity is high at ... dust opacity at 60 of 228 cm gr the best model for OH44.8 has the following ... dust located very near the photosphere --- is directly detected at wavelengths as ...
... and not all galaxies that show such structures have detectable HI or obvious dust ... Centaurus A. In addition to its distinctive dust lanes, it has an extensive low ...
... have already observed molecular gas and dust in a handful of high redshift radio ... CO content implied an equally enormous amount of dust but this has not so far been ...
... dust continuum and HCO + ( J =1-0) line emission at 89 GHz (3.4 mm) from two young southern disk targets, TW Hya, the closest known classical T Tauri star, and HD 100546, a nearby Herbig Be star whose infrared spectrum shows crystalline silicates ...
... dust attenuation which extends up to 40 (1.9 kp c) ab ove the plane of the galaxy ... dust structures can be located and identified (Howk & Savage 2000) and it is natural ...
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Ссылки http://www.atnf.csiro.au/people/Peter.Kamphuis/Thesis/ch3.pdf -- 543.8 Кб -- 21.10.2013 Похожие документы