On the structure of the transition disk around TW Hydrae

Context. For over a decade, the structure of the inner cavity in the transition disk of TW Hydrae has been a subject of debate. Modeling the disk with data obtained at different wavelengths has led to a variety of proposed disk structures. Rather than being inconsistent, the individual models might...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2014-04, Vol.564, p.np-np
Hauptverfasser:	Menu, J., van Boekel, R., Henning, Th, Chandler, C. J., Linz, H., Benisty, M., Lacour, S., Min, M., Waelkens, C., Andrews, S. M., Calvet, N., Carpenter, J. M., Corder, S. A., Deller, A. T., Greaves, J. S., Harris, R. J., Isella, A., Kwon, W., Lazio, J., Le Bouquin, J.-B., Ménard, F., Mundy, L. G., Pérez, L. M., Ricci, L., Sargent, A. I., Storm, S., Testi, L., Wilner, D. J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Density Disks Dust Fittings Grains Interferometry Physics Planet formation protoplanetary disks stars: individual: TW Hya techniques: interferometric Wavelengths
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