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Dust Properties of Protoplanetary Disks in the Taurus-Auriga Star Forming Region from Millimeter Wavelengths
L. Ricci, L. Testi, A. Natta +3
We present the most sensitive 3 mm-survey to date of protoplanetary disks carried in the Taurus-Auriga star forming region (average rms of about 0.3 mJy), using the IRAM PdBI. With…
Strong near-infrared emission in the sub-AU disk of the Herbig Ae star HD163296: evidence for refractory dust?
M. Benisty, A. Natta, A. Isella +12
We present new long-baseline spectro-interferometric observations of the HerbigAe star HD163296 obtained in the H and K bands with the AMBER instrument at VLTI. The observations co…
Results from DROXO. II. - [Ne II] and X-ray emission from Rho Ophiuchi young stellar objects
E. Flaccomio, B. Stelzer, S. Sciortino +3
The infrared [Ne II] and [Ne III] fine structure lines at 12.81um and 15.55um are predicted to trace the circumstellar disk gas subject to X-ray heating and ionization. We investig…
Resolving the molecular environment of Super Star Clusters in Henize 2-10
G. Santangelo, L. Testi, L. Gregorini +4
The rate of star formation both in the Galaxy and in external galaxies should be related to the physical properties of the molecular clouds from which stars form. This is expected…
Properties of Stellar Clusters around High-Mass Young Stars
Fabiana Faustini, Sergio Molinari, Leonardo Testi +1
[Abridged] Twenty-six high-luminosity IRAS sources believed to be collection of stars in the early phases of high-mass star formation have been observed in the NIR (J, H, K) to cha…
ATLASGAL - The APEX Telescope Large Area Survey of the Galaxy at 870 microns
F. Schuller, K. M. Menten, Y. Contreras +31
(Abridged) Studying continuum emission from interstellar dust is essential to locating and characterizing the highest density regions in the interstellar medium. In particular, the…