Year: 2011
Type: article
Abstract: Context. We present the results of the analysis of low-resolution optical-near IR spectroscopy (0.6–2.4 μm) of a sample (47 sources) of Class I and Class II young stellar objects in the Chamaeleon I and II star-forming clouds. These data are part of the POISSON project (Protostellar Optical-Infrared Spectral Survey On NTT).
Source: Astronomy and Astrophysics
Institutions: Astronomical Observatory of Rome, National Institute for Astrophysics, Max Planck Institute for Radio Astronomy, Thüringer Landessternwarte Tautenburg, Arcetri Astrophysical Observatory, Centre National de la Recherche Scientifique, Observatoire de Paris, École Normale Supérieure - PSL, Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et Atmosphères, Université Pierre-et-Marie-Curie, Dublin Institute For Advanced Studies, Institut de Planétologie et d'Astrophysique de Grenoble
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W4291007615