Variable accretion as a mechanism for brightness variations in T Tauri S

The southern “infrared companion” of T Tau is known to show strong photometric variations of several magnitudes on timescales of years, as well as more modest 1 mag variations on timescales as short as one week. The physical mechanism driving these variations is debated, intrinsic luminosity variati...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Boekel, Roy van (VerfasserIn) , Juhász, A. (VerfasserIn) , Henning, Th (VerfasserIn) , Köhler, Rainer (VerfasserIn) , Ratzka, Th (VerfasserIn) , Herbst, T. (VerfasserIn) , Bouwman, J. (VerfasserIn) , Kley, W. (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 26 July 2010
In: Astronomy and astrophysics
Year: 2010, Jahrgang: 517, Pages: 1-15
ISSN:1432-0746
DOI:10.1051/0004-6361/200913840
Online-Zugang:Resolving-System, lizenzpflichtig, Volltext: https://doi.org/10.1051/0004-6361/200913840
Verlag, lizenzpflichtig, Volltext: https://www.aanda.org/articles/aa/abs/2010/09/aa13840-09/aa13840-09.html
Volltext
Verfasserangaben:R. van Boekel, A. Juhász, Th. Henning, R. Köhler, Th. Ratzka, T. Herbst, J. Bouwman, and W. Kley
Beschreibung
Zusammenfassung:The southern “infrared companion” of T Tau is known to show strong photometric variations of several magnitudes on timescales of years, as well as more modest 1 mag variations on timescales as short as one week. The physical mechanism driving these variations is debated, intrinsic luminosity variations due to a variable accretion rate were initially proposed, but later challenged in favor of apparent fluctuations due to time-variable foreground extinction. We seek to investigate the nature of the observed photometric variability. Based on simple geometric arguments and basic physics laws, a minimum variability timescale can be derived for which variable extinction is a viable mechanism. Because this timescale increases rapidly with wavelength, observations at long wavelengths provide the strongest constraints.
Beschreibung:Gesehen am 29.08.2023
Beschreibung:Online Resource
ISSN:1432-0746
DOI:10.1051/0004-6361/200913840