On the nature of the spectrum veiling for classical T Tauri stars in the near infrared

We show that the presence of a hot accretion spot on the surface of classical T Tauri stars allows the observed veiling of their photospheric spectrumto be explained not only in the visible but also in the near infrared.

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Bibliographische Detailangaben
Veröffentlicht in:	Astronomy letters 2013-06, Vol.39 (6), p.389-392
Hauptverfasser:	Dodin, A. V., Lamzin, S. A.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion Astronomy Astrophysics Astrophysics and Astroparticles Infrared radiation Observations and Techniques Physics Physics and Astronomy Stars & galaxies
Online-Zugang:	Volltext
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Beschreibung
Zusammenfassung:	We show that the presence of a hot accretion spot on the surface of classical T Tauri stars allows the observed veiling of their photospheric spectrumto be explained not only in the visible but also in the near infrared.
ISSN:	1063-7737 1562-6873
DOI:	10.1134/S1063773713060042