Binary-object spectral-synthesis in 3D (BOSS-3D) -- Modelling H-alpha emission in the enigmatic multiple system LB-1

Context: To quantitatively decode the information stored within an observed spectrum, detailed modelling of the physical state and accurate radiative transfer solution schemes are required. In the analysis of stellar spectra, the numerical model often needs to account for binary companions and 3D st...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	arXiv.org 2021-11
Hauptverfasser:	Hennicker, L, Kee, N D, Shenar, T, Bodensteiner, J, Abdul-Masih, M, I El Mellah, Sana, H, Sundqvist, J O
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Astronomical models B stars Binary stars Coordinate transformations Deposition H alpha line Numerical models Physics - Solar and Stellar Astrophysics Planetary atmospheres Radiative transfer Stellar envelopes Stellar spectra Stellar winds Synthesis Three dimensional models
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!