Protostars, multiplicity, and disk evolution in the Corona Australis region: aHerschelGould Belt Study
Year: 2012
Type: article
Abstract: Context. The CrA region and the Coronet cluster form a nearby (138 pc), young (1−2 Myr) star-forming region that hosts a moderate population of Class I, II, and III objects.
Source: Astronomy and Astrophysics
Institutions: Universidad Autónoma de Madrid, Max Planck Institute for Astronomy, Centre National de la Recherche Scientifique, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Astrophysique, Instrumentation et Modélisation, CEA Paris-Saclay, Institut de Recherche sur les Lois Fondamentales de l'Univers, Université Paris Diderot, Rutherford Appleton Laboratory, The Open University
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
Funders: National Science Foundation, National Aeronautics and Space Administration, California Institute of Technology, Centre National d’Etudes Spatiales, KU Leuven, Ministerio de Ciencia e Innovación, Bundesministerium für Verkehr, Innovation und Technologie, Max-Planck-Institut für Astronomie, Science and Technology Facilities Council
OpenAlex ID: W2070126479