The intrinsic reddening of the Magellanic Clouds as traced by background galaxies: I. The bar and outskirts of the Small Magellanic Cloud

ABSTRACT. We present a method to map the total intrinsic reddening of a foreground extinguishing medium via the analysis of spectral energy distributions (SEDs

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Bibliographische Detailangaben
Hauptverfasser: Bell, Cameron P. M. (VerfasserIn) , Martínez-Delgado, David (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 2019 August 23
In: Monthly notices of the Royal Astronomical Society
Year: 2019, Jahrgang: 489, Heft: 3, Pages: 3200-3217
ISSN:1365-2966
DOI:10.1093/mnras/stz2325
Online-Zugang:Verlag, Volltext: https://doi.org/10.1093/mnras/stz2325
Verlag: https://academic.oup.com/mnras/article/489/3/3200/5553996
Volltext
Verfasserangaben:Cameron P.M. Bell, Maria-Rosa L. Cioni, A.H. Wright, Stefano Rubele, David L. Nidever, Ben L. Tatton, Jacco Th. van Loon, Valentin D. Ivanov, Smitha Subramanian, Joana M. Oliveira, Richard de Grijs, Clara M. Pennock, Yumi Choi, Dennis Zaritsky, Knut Olsen, Florian Niederhofer, Samyaday Choudhury, David Martínez-Delgado and Ricardo R. Muñoz
Beschreibung
Zusammenfassung:ABSTRACT. We present a method to map the total intrinsic reddening of a foreground extinguishing medium via the analysis of spectral energy distributions (SEDs
Beschreibung:Gesehen am 08.10.2019
Beschreibung:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stz2325