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- W3153405944 abstract "Interferometry at (sub)mm wavelengths is one of the most important tools to study the physical and chemical properties of the youngest and most embedded stages of star formation. High spatial resolution is needed to resolve small scale structure e.g. details of accretion disks or molecular outflows and the sub(mm) wavelength bands are important because the young and deeply embedded stages of star formation are characterized by cold gas and dust temperatures of the order of 10K. In this article I will discuss some of the most important applications of sub(mm) interferometry and in addition I will give an overview of the sub(mm) array ALMA." @default.
- W3153405944 created "2021-04-26" @default.
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- W3153405944 date "2008-01-01" @default.
- W3153405944 modified "2023-09-27" @default.
- W3153405944 title "Sub)mm Interferometry Applications in Star Formation Research" @default.
- W3153405944 hasPublicationYear "2008" @default.
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