The inner circumstellar disk of the UX Orionis star V1026 Scorpii

Context. The UX Ori type variables (named after the prototype of their class) are intermediate-mass pre-main sequence objects. One of the most likely causes of their variability is the obscuration of the central star by orbiting dust clouds. Aims. We investigate the structure of the circumstellar en...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2014-04, Vol.564, p.np-np
Hauptverfasser:	Vural, J., Kreplin, A., Kishimoto, M., Weigelt, G., Hofmann, K.-H., Kraus, S., Schertl, D., Dugué, M., Duvert, G., Lagarde, S., Massi, F.
Format:	Artikel
Sprache:	eng
Schlagworte:	accretion accretion disks Astronomy Astrophysics circumstellar matter Clouds Disks Dust Inclination Sciences of the Universe Spectral energy distribution Stars stars: formation stars: individual: V1026 Sco stars: pre-main sequence techniques: interferometric Visibility
Online-Zugang:	Volltext
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