J. F. Albacete Colombo

TL;DR: In this article, the authors present a list of the institutions of interest in the field of astronomy, including the Smithsonian Astrophysical Observatory, Cambridge, USA, Department of Physics & Astronomy, University College London, United Kingdom (4) Centro regional Zona Atlantica, Universidad Nacional del Comahue, Viedma, Argentina (5) Instituto de AstrofA±sica de Canarias (IASCA), Universidad de La Laguna, Spain (6) University of Wyoming, Laramie, USA (7

TL;DR: In this paper, the authors performed a multi-wavelength study of the SNR G18.1-0.1 and nearby several HII regions (infrared dust bubbles N21 and N22, and the HII region G018.149-00.181) and showed that the objects analysed in this work belong to a same complex located at the distance of about 4 kpc.

TL;DR: Combi et al. as mentioned in this paper presented a paper on radioastronomia at the Universidad Nacional de la Plata (Universidad de Jaen) in Argentina.

TL;DR: In this paper, the Eta Chamaleontis cluster members were determined in terms of coronal temperature, column density, emission measure, X-ray luminosity and variability.

TL;DR: In this paper, the authors used the wavelet-based code PWDetect to detect sources in the composed EPIC pn+mos image, and determined both the coronal properties and variability of the η Chamaleontis members in the XMM-Newton EPIC field-of-view.