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ALMA observations of cool dust in a low-metallicity starburst, SBS0335-052
L. K. Hunt, L. Testi, V. Casasola +9
We present Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 0 Band 7 observations of an extremely metal-poor dwarf starburst galaxy in the Local Universe, SBS0335-052 (12+…
The ATLASGAL survey: a catalog of dust condensations in the Galactic plane
T. Csengeri, J. S. Urquhart, F. Schuller +10
The formation processes and the evolutionary stages of high-mass stars are poorly understood compared to low-mass stars. Large-scale surveys are needed to provide an unbiased censu…
Silicon isotopic abundance toward evolved stars and its application for presolar grains
T. -C. Peng, E. M. L. Humphreys, L. Testi +8
Galactic chemical evolution (GCE) is important for understanding the composition of the present-day interstellar medium (ISM) and of our solar system. In this paper, we aim to trac…
On the shape of the mass-function of dense clumps in the Hi-GAL fields. II. Using Bayesian inference to study the clump mass function
L. Olmi, D. Angles-Alcazar, D. Elia +6
Context. Stars form in dense, dusty clumps of molecular clouds, but little is known about their origin, their evolution and their detailed physical properties. In particular, the r…
A UV-to-MIR monitoring of DR Tau: exploring how water vapor in the planet formation region of the disk is affected by stellar accretion variability
Andrea Banzatti, Michael R. Meyer, Carlo F. Manara +2
Young stars are known to show variability due to non-steady mass accretion rate from their circumstellar disks. Accretion flares can produce strong energetic irradiation and heatin…
A Community Science Case for E-ELT HIRES
R. Maiolino, M. Haehnelt, M. T. Murphy +57
Building on the experience of the high-resolution community with the suite of VLT high-resolution spectrographs, which has been tremendously successful, we outline here the (scienc…