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We apply Support Vector Machines -- a machine learning algorithm -- to the task of classifying structures in the Interstellar Medium. As a case study, we present a position-position velocity data cube...
The ISM, powered by SNe, is turbulent and permeated by a magnetic field (with a mean and a turbulent component). It constitutes a frothy medium that is mostly out of equilibrium and is ram pressure do...
The fate of metals after they are released in starburst episodes is still unclear. What phases of the interstellar medium are involved, in which timescales?
We analyse SPI/INTEGRAL data on the 511 keV line from the Galactic Centre, accumulated over ~6 years of observations.
We present the results of the search for candidate Planetary Nebulae interacting with the interstellar medium (PN-ISM) in the framework of the INT Photometric H$\alpha$ Survey (IPHAS) and located in t...
Diagnostics of the Ionized ISM:The Importance of Density Fluctuations。
HD 192281 and HD 10125:A Study of their Local ISM using Radio and Infrared Data。
Photoionizing shocks in the ISM     ISM  Photoionizing shocks       2009/6/8
Photoionizing shocks in the ISM
A High Resolution H I Study of the ISM Local to Galactic Wolf-rayet Stars。
The dependence of the thermal pressure of hot galactic halos on a model parameter describing the frequency of major reheating episodes during galactic history is investigated. Pressure on the interf...

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