Hallo Caro,
<blockquote id="quote"><font size="1" face="Verdana, Arial, Helvetica" id="quote">Zitat:<hr height="1" noshade id="quote"><i>Original erstellt von: Caro</i>
<br /> Ich habe so das Gefühl, das hat man beim VLT damals überschätzt. Interferometrie ist in gewisser Weise "out" und wird einfach nicht so häufig verwendet. <hr height="1" noshade id="quote"></blockquote id="quote"></font id="quote">
Erstaunlich, angesichts der erzielbaren Auflösung:
http://www.eso.org/sci/facilit…escopes/vlti/science.html
<blockquote id="quote"><font size="1" face="Verdana, Arial, Helvetica" id="quote">Zitat:<hr height="1" noshade id="quote">YSOs offer a rich circumstellar environment such as accretion disks, stellar companions, optical jets, stellar winds and show a variety of different phenomena like infrared excesses, luminosity variations and highly collimated jets. Most of these phenomena occur in a region with a size less than 1 AU. Long-baseline optical interferometry, with its milliarcsecond (mas) resolution typically corresponding to 0.1 AU at 100 pc is particularly suitable to probe the physical processes and interactions of the early stages of star and planet formation.<b></b><hr height="1" noshade id="quote"></blockquote id="quote"></font id="quote">
Dank auch an Kalle.
