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

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Bibliographic Details
Main Authors:	Weber, Michael L. (Author) , Ercolano, Barbara (Author) , Picogna, Giovanni (Author) , Hartmann, Lee (Author) , Rodenkirch, Peter (Author)
Format:	Article (Journal)
Language:	English
Published:	2020 June 3
In:	Monthly notices of the Royal Astronomical Society Year: 2020, Volume: 496, Issue: 1, Pages: 223-244
ISSN:	1365-2966
DOI:	10.1093/mnras/staa1549
Online Access:	Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/staa1549 Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/496/1/223/5850787
Author Notes:	Michael L. Weber, Barbara Ercolano, Giovanni Picogna, Lee Hartmann and Peter J. Rodenkirch

Description
Summary:	ABSTRACT. High-resolution spectra of typical wind diagnostics ([O i] 6300 Å and other forbidden emission lines) can often be decomposed into multiple component
Item Description:	Gesehen am 17.09.2020
Physical Description:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/staa1549