Cargando…
Water in the terrestrial planet-forming zone of the PDS 70 disk
Terrestrial and sub-Neptune planets are expected to form in the inner (less than 10 au) regions of protoplanetary disks(1). Water plays a key role in their formation(2–4), although it is yet unclear whether water molecules are formed in situ or transported from the outer disk(5,6). So far Spitzer Sp...
Autores principales: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
---|---|
Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group UK
2023
|
Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10432267/ https://www.ncbi.nlm.nih.gov/pubmed/37488359 http://dx.doi.org/10.1038/s41586-023-06317-9 |