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Using Hubble Space Telescope (HST) photometry, we characterize the age of the stellar association in the vicinity of supernova (SN) 2011dh and use it to infer the zero-age main sequence mass (M_{ZAMS}...
We present an observational study towards the young high-mass star forming region G23.44-0.18 using the Submillimeter Array. Two massive, radio-quiet dusty cores MM1 and MM2 are observed in 1.3 mm con...
We analyze the dependence of galaxy structure (size and Sersic index) and mode of star formation (\Sigma_SFR and SFR_IR/SFR_UV) on the position of galaxies in the SFR versus Mass diagram. Our sample c...
We present near-infrared JHKs imaging as well as K-band multi-object spectroscopy of the massive stellar content of W3 Main using LUCI at the LBT. We confirm 13 OB stars by their absorption line spect...
Quasar Optical Variability and Black Hole Mass
Analisys of the luminosity-stellar mass-metallicity relation in cosmological simulations。
Big game hunting in the andromeda galaxy:identifying And weighing black holes in low mass x-ray binaries。
Orbital Dynamics Analysis of Binary Systems in Mass-Loss Scenarios。
The Partition Between Terminal Speed and Mass Loss:Thin, Thick, and Rotating Line-Driven Winds。
Parsec-Scale Outflows from Intermediate-Mass Stars。
A spherically symmetric mass distribution with two scale parameters for the dark corona of a (spiral) galaxy as an alternative to the usually applied quasi-isothermal sphere is considered. Examinati...

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