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The Effect of External Photoevaporation on the Disk Fraction in M17
Samuel Millstone, Megan Reiter, Morten Andersen +6
A major obstacle to improving models of planet formation is understanding how the local environment influences the lifetime of the disks in which they form. The spread in observed…
Spectral classification of young stars using conditional invertible neural networks II. Application to Trumpler 14 in Carina
Da Eun Kang, Dominika Itrich, Victor F. Ksoll +3
We introduce an updated version of our deep learning tool that predicts stellar parameters from the optical spectra of young low-mass stars with intermediate spectral resolution. W…
The past, present and future of observations of externally irradiated disks
Planet formation environments collaboration, Megan Allen, Rossella Anania +51
Recent years have seen a surge of interest in the community studying the effect of ultraviolet radiation environment, predominantly set by OB stars, on protoplanetary disc evolutio…
The population of young low-mass stars in Trumpler 14
Dominika Itrich, Leonardo Testi, Giacomo Beccari +8
Massive star-forming regions are thought to be the most common birth environments in the Galaxy and the only birth places of very massive stars. Their presence in the stellar clust…
Spectral classification of young stars using conditional invertible neural networks I. Introducing and validating the method
Da Eun Kang, Victor F. Ksoll, Dominika Itrich +4
Aims. We introduce a new deep learning tool that estimates stellar parameters (such as effective temperature, surface gravity, and extinction) of young low-mass stars by coupling t…
The Herschel-PACS legacy of low-mass protostars: Properties of warm and hot gas and its origin in far-UV illuminated shocks
Agata Karska, Michael J. Kaufman, Lars E. Kristensen +11
Recent observations from Herschel allow the identification of important mechanisms responsible for the heating of gas surrounding low-mass protostars and its subsequent cooling in…