The interpretation of protoplanetary disc wind diagnostic lines from X-ray photoevaporation and analytical MHD models
ABSTRACT. High-resolution spectra of typical wind diagnostics ([O i] 6300 Å and other forbidden emission lines) can often be decomposed into multiple component
Gespeichert in:
| Hauptverfasser: | , , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2020 June 3
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2020, Jahrgang: 496, Heft: 1, Pages: 223-244 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/staa1549 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/staa1549 Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/496/1/223/5850787 
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| Verfasserangaben: | Michael L. Weber, Barbara Ercolano, Giovanni Picogna, Lee Hartmann and Peter J. Rodenkirch |
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