We present combined information on the optical morphology derived from HST images and the infrared properties of the dust in the circumstellar envelope derived...

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We present a preliminary analysis of ISO-SWS spectra of a sample of Vega-type and pre-main sequence stars, which were observed from the ground in a project...

Dwarf galaxies in the Local Group allow to study in great detail the physical mechanisms responsible for the formation and evolution of galaxies. In fact, their...

Studying the birthplaces of massive stars is crucial for understanding the role of clustering in the formation of these objects. Some authors claim that massive...

Most accretion-powered relativistic jet sources in our Galaxy are transient X-ray binaries (XBs). Efforts to coordinate multiwavelength observations of these...

ISOPHOT, the imaging spectro-photo-polarimeter on board ISO, supported performance of aperture and mapping photometry, low-resolution spectroscopy and...

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As part of the ISO calibration programme, we observed the mid-infrared spectrum of the Zodiacal Light at low and high ecliptie latitudes, using the...