Year: 2014
Type: article
Abstract: Context. Investigating the evolution of protoplanetary disks is crucial for our understanding of star and planet formation. There have been several theoretical and observational studies in past decades to advance this knowledge. The launch of satellites operating at infrared wavelengths, such as the Spitzer Space Telescope and the Herschel Space Observatory, has provided important tools for investigating the properties of circumstellar disks.
Source: Astronomy and Astrophysics
Institutions: ETH Zurich, Arcetri Astrophysical Observatory, University of Groningen, Centre National de la Recherche Scientifique, Université Joseph Fourier, Institut de Planétologie et d'Astrophysique de Grenoble, University of Chile, Clemson University, Universidad Autónoma de Madrid, Centro de Astrobiología, University of Vienna, University of St Andrews, Royal Observatory, UK Astronomy Technology Centre
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
Awards: G1323383031, WE SEEK SUPPORT TO HOMOGENEOUSLY REDUCE AND ANALYZE ARCHIVAL SPITZER/IRS SPECTRA FOR A SAMPLE OF 147, G2325242462, G2861369480, G3207356259, G393177772, G4104599821, Interferometry in the near-infrared: a very high angular resolution insight into the accretion/ejection process in young stars, Astronomy Fellowships in Italy, G5702163051, Analysis and Modelling of Multi-wavelength Observational Data from Protoplanetary Discs
OpenAlex ID: W2065207649